The galaxy appears as a somewhat smooth, elliptical-like structure. Its color exhibits a generally yellowish hue, suggestive of an older stellar population. There are hints of possible minor disturbances or interactions, which could be indicative of past or ongoing minor merging activity. The light is fairly concentrated toward the center, appearing fairly uniformly distributed throughout. Overall, the galaxy is observed to be an early-type system with a relatively high degree of central concentration and is likely a fairly massive galaxy with very little star formation.
