The galaxy presents as an elliptical, slightly cigar-shaped structure. It exhibits a smooth, relatively featureless morphology with a highly concentrated central bulge. The core region appears bright and yellowish in color, suggesting a population of older stars. There is no visible spiral arm structure or dust lanes. The galaxy displays a gradual decrease in luminosity from the center outward, transitioning to a fainter, diffuse halo. There is no indication of ongoing major merging activity, though there is some minor disruption of the galaxy, there is a slight distortion in its overall shape, possibly indicating a past or minor interaction with another galaxy. Overall the smooth, featureless appearance suggests a relatively evolved system with a moderate amount of star formation.
