The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and concentrated light profile. It shows a distinct central bulge, characterized by a yellow-orange hue, indicative of an older stellar population. Fainter, bluer regions surround the core, which could suggest some level of recent star formation. The overall shape is somewhat elongated, but not highly flattened; it presents as neither perfectly round nor highly elongated. There is no clear evidence of spiral arms or a well-defined disk structure. There is no strong evidence of tidal tails or significant morphological distortions, suggesting it is not currently undergoing a major merger. It displays a minor amount of disturbance, but is mostly undisturbed.
