The galaxy presents as a roughly elliptical, relatively smooth object. A bright central bulge is observed, exhibiting a yellowish hue, suggesting a population of older stars. The galaxy appears to fade gradually from its core, with a minimal amount of visible structure or spiral arms. Its overall shape is between round and elliptical. There may be a hint of a faint disk component. There is no evidence of major interaction or merging activity. Based on the color gradient, the galaxy's star formation rate seems to be relatively low.
