The galaxy appears to be a relatively smooth, elliptical galaxy, possibly an early-type spiral galaxy. It exhibits a bright central bulge, surrounded by a fainter, more diffuse halo or disk-like structure. The color profile suggests a population of older stars, given the slightly reddish hue emanating from the outer regions. The galaxy's light distribution seems somewhat elongated. There may be some minor disturbances in the light distribution, suggesting potential interactions or past merger events. While the galaxy is predominantly smooth, there's a hint of a possible disk or arm-like structure, though it is not clearly defined.
