The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated, with a gradual decrease in luminosity outward. The galaxy exhibits a subtle elongation, with a roughly in-between shape of being circular or cigar shaped. There is a slight indication of a disk-like structure, although the primary visual characteristic is that of a smooth, featureless object. There appears to be no current or recent major merger activity influencing the overall morphology of the galaxy. The central region has a yellowish hue, potentially indicative of an older stellar population. The outer regions exhibit a more diffuse and somewhat redder color, possibly from dust or a population of older stars. There may be low levels of on-going star formation. The galaxy has intermediate luminosity.
