The galaxy presents a generally elliptical morphology, exhibiting a relatively smooth and concentrated light distribution. The core region is characterized by a bright, slightly elongated central bulge, indicating a high density of stars. The overall color is predominantly redder, shifting into yellow, suggesting an older stellar population with a lower rate of ongoing star formation. There is a subtle hint of a disk-like structure, although it is not sharply defined. There may be some minor dust lanes or faint spiral features that cause slight irregularities in the light distribution.
