The galaxy presents as a relatively smooth, elliptical-like morphology. It appears elongated, approximately a 3:1 ratio in its major to minor axis. The central region exhibits a higher concentration of light, indicating a prominent bulge. The outer regions show a gradual decrease in luminosity, with no discernible spiral arm structures or significant dust lanes visible.

The color profile suggests a relatively old stellar population, particularly in the bulge. The overall color is slightly redder in the core, grading to bluer hues in the outer regions, suggesting that there may be ongoing, but moderate, star formation.

There is no clear evidence of any major tidal disturbances or ongoing mergers, although some minor asymmetry could suggest past interactions.
