The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical in projection. The color profile suggests a dominant population of older stars, contributing to its yellowish-orange hue. There is very little visual evidence of ongoing star formation within the galaxy based on the color. Faint diffuse light extends outwards from the central region, gradually fading into the background sky. No prominent spiral arms, dust lanes, or other distinct features are immediately apparent, indicating a relatively undisturbed and dynamically settled system. The galaxy lacks any obvious signs of tidal interactions or merging events, although there may be signs of minor disturbance based on its asymmetry.
