The galaxy presents as a single, relatively smooth object. The overall shape appears elliptical, exhibiting a slight elongation, but largely tending toward roundness. It shows a high degree of central concentration with a bright core region that fades gradually into the outer parts. The color profile suggests a somewhat evolved stellar population, appearing more yellow/red in composition than blue, indicative of older stars. There's no obvious presence of significant spiral arm structure or dust lanes. There may be evidence of some minor gravitational disturbance or interaction, but it is not overtly merging with another galaxy, nor strongly disrupted.
