The galaxy presents as a relatively smooth, elongated structure. The central region exhibits a brighter, more concentrated luminosity, suggesting a substantial stellar population and possibly a supermassive black hole at its core. Moving outwards from the center, the light gradually diminishes.

The galaxy displays a subtle color gradient. The core appears more reddish or yellowish. The outer regions show a bluer hue. This color difference could be indicative of varying stellar populations, with older, redder stars dominating the core and younger, bluer stars located further out, or dust obscuring the central parts.

The overall morphology appears relatively undisturbed, without prominent tidal tails or other signs of recent major mergers or interactions. There is a slight asymmetry. Overall, this object appears to be an elliptical galaxy.
