The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a roughly elliptical morphology, appearing quite rounded. The light distribution suggests a centrally dominant bulge with a gradual decrease in luminosity outwards.

There is no obvious spiral structure or prominent dust lanes visible, and the overall color is indicative of an older stellar population, with a possible lack of significant ongoing star formation. There are subtle irregularities visible in the outer regions, though the light is too faint to make definitive judgement.
