This galaxy presents as a moderately compact, yet slightly diffuse object. The central region exhibits a bright, concentrated core. Moving outwards, there is a noticeable shift in color and intensity.

The overall color profile suggests active star formation within the galaxy, specifically indicated by a distinct blue-green hue. This hue appears to be concentrated in and around the central core, potentially indicating a higher density of younger, hotter stars in this region. The outer reaches display a shift towards warmer tones, likely indicative of an older stellar population or dust obscuration.

The overall morphology appears to be somewhat disturbed, with no clear spiral arm structure readily apparent. There are subtle irregularities and extensions, suggesting possible past interactions with other galaxies, or internal dynamical processes at play. This object may be in the early stages of a merger, and exhibits characteristics that suggest a complex evolutionary history.
