The galaxy presents as a single, moderately bright object with a relatively smooth light distribution. The overall morphology appears to be elliptical or lenticular, exhibiting a high degree of central concentration. The light profile suggests a lack of significant spiral arm structure or prominent dust lanes. There appears to be a small amount of asymmetry that could be consistent with a minor gravitational interaction. The object's color is notably redder than average, implying an older stellar population and a relatively low rate of ongoing star formation. There is a possible secondary core indicating a merger may have occurred in the past or is currently in the process of happening. The apparent size of the galaxy is relatively small, suggestive of a considerable distance.
