The galaxy appears to be an elliptical galaxy, with a generally smooth and concentrated light distribution. It presents with a moderately elongated shape, not perfectly spherical. There is a bright central bulge, which gradually fades into the outer regions. The color gradient suggests the presence of older stellar populations. There is no clear evidence of spiral arms or prominent dust lanes, and only minor indications of disturbance. The galaxy appears relatively isolated and exhibits limited signs of any ongoing major merging events. The general features suggest that star formation is low.
