This galaxy appears to be a relatively smooth, elliptical galaxy, exhibiting a concentrated central bulge. There is some evidence of a slight deviation from perfect sphericity, but it does not appear elongated. No prominent spiral arm structures are visible. There is a color gradient, shifting from yellowish hues at the core to bluish tones at the periphery, suggesting a distribution of stellar populations, with older stars concentrated towards the center. There is no clear indication of major disturbances from mergers, but the slight irregularities in shape suggest a minor disturbance could be present.