This galaxy appears to be a relatively smooth, elliptical system. It exhibits a centrally concentrated light profile, with luminosity decreasing gradually outwards from a bright core. The overall shape approximates a slightly elongated spheroid, showing minimal evidence of a disk structure. The color gradient suggests a population of older stars, with a yellowish-red hue dominating throughout. There is no clear indication of significant star formation activity or the presence of spiral arms. The galaxy's morphology suggests it is a mature system, possibly residing in a relatively dense environment.
