The galaxy presents a moderately resolved structure, appearing as a relatively compact system. The light profile suggests a primary spheroidal component, with a smooth, centralized concentration of stellar mass. The distribution of light, however, exhibits asymmetry, indicating a deviation from a perfect elliptical shape. This could be indicative of tidal interactions or past mergers.

A secondary, bluer component is visible, displaced from the main body. The color suggests ongoing star formation within this region. It is unclear if this is simply a star forming region within the galaxy, or perhaps an interacting companion.

There is some visual evidence of minor disturbances in the overall morphology, possibly resulting from interactions. There is no strong visual evidence to support a major ongoing merger, but a faint tidal tail, or asymmetry in the outer isophotes of the main body cannot be excluded.

The dominant color of the galaxy, beyond the bluer area, is somewhat redder, which might indicate an older stellar population dominating the light output. The overall luminosity is significant, implying a galaxy of substantial stellar mass.
