The galaxy presents as a relatively smooth, elliptical object. It exhibits a concentrated central bulge that appears nearly spherical and emits a significant amount of light, suggesting a high density of stars within this region. The light profile decreases gradually from the center towards the outer edges of the galaxy, indicating a diffuse halo. There's a slight elongation, though it doesn't classify as a spiral galaxy due to the absence of distinct spiral arms. There's no sign of significant dust lanes or patchy star formation regions. Based on the light distribution and overall morphology, it appears to be an evolved system with a relatively old stellar population. There are hints of minor gravitational disturbances and possibly interaction with other smaller objects.
