The galaxy presents as a largely smooth, elliptical-like structure. It appears highly symmetrical and concentrated, with a bright central bulge that dominates its overall luminosity. There is a subtle color gradient observable, shifting from a slightly bluer hue in the outer regions to a redder, yellower core. There is no clearly defined disk structure or spiral arms visible; the light distribution appears relatively uniform throughout the galaxy's body, suggestive of an older stellar population with minimal ongoing star formation. There appears to be very minor morphological disturbance in the form of a slight elongation to one side of the galaxy. There is no evidence of significant tidal features or interactions with other galaxies that would indicate it is in the process of merging. Overall, this galaxy appears to be a relatively undisturbed, mature system.
