The galaxy presents a predominantly smooth morphology, exhibiting a concentrated central bulge. There is minimal evidence of spiral arm structure or prominent dust lanes. The overall shape is largely round with some elongation. There appears to be a very subtle disturbance or a tidal feature on the lower right, suggesting a possible interaction or minor merger in its past, or perhaps a small satellite galaxy is interacting with the primary galaxy. The galaxy is strongly concentrated centrally and fades gradually towards its outer edges, with no other bright knot of activity. The color appears relatively uniform across the galaxy, indicating a lack of significant star forming regions. The lack of distinct features suggests an older stellar population.
