The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a notable central bulge that is the brightest region, suggesting a high concentration of stars towards the galactic center. The overall color appears yellowish-white, which is indicative of an older stellar population. The galaxy appears somewhat elongated, deviating from a perfectly circular shape. There is no clear evidence of spiral arm structures or significant dust lanes. Faint extensions or disturbances are subtly apparent, indicating some tidal interaction or recent merger event, however the overall morphology suggests it is not currently undergoing any major mergers.
