The galaxy presents a generally smooth morphology, with a slightly elliptical shape. It exhibits a concentrated central bulge. The color appears to be a warm yellow-orange hue, indicative of an older stellar population with fewer actively forming stars. There is a potential secondary object in close proximity, possibly interacting or in the process of merging with the primary galaxy. The galaxy appears relatively undisturbed with no prominent tidal tails or strong distortions, yet the possibility of minor disturbances is present. Overall, the galaxy gives the impression of being a fairly massive, evolved system, with the suggestion of ongoing or recent interactions.
