The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a gradual decline in brightness towards its outer regions. The galaxy appears predominantly featureless, lacking prominent spiral arms or strong dust lanes. There may be subtle disturbances. The galaxy's overall shape is roughly circular. Color analysis reveals a general red hue, suggestive of an older stellar population with a relatively low rate of ongoing star formation. The galaxy appears to be a significant mass, though not the most massive.
