The galaxy presents a smooth, elliptical morphology with a slight cigar-like elongation. The color gradient suggests a centrally concentrated population of older stars, indicated by the reddish hue in the core region. Fainter, bluer emission is present in the outer regions, suggestive of ongoing, albeit low-level, star formation. There is no strong indication of spiral arms or a prominent disk structure. The galaxy exhibits no significant signs of tidal disturbances or ongoing major mergers. There appears to be some minor interaction occurring, with slightly asymmetrical features.
