The galaxy presents as a relatively compact, elliptical-like structure with a smooth, diffuse appearance. The central region is brighter and more concentrated than the outer regions. The light distribution gradually decreases with distance from the center, indicative of an older stellar population. There's some slight evidence of asymmetry or minor disturbance in the galaxy's shape, possibly hinting at a past or ongoing interaction. Faint features are visible that may indicate the presence of a very weak disk structure. The color of the galaxy appears yellowish-orange, suggesting a population dominated by older, redder stars. Star formation appears to be low. Overall the galaxy seems to be a fairly massive and quiescent object.
