The galaxy presents as a centrally concentrated, elliptical morphology. The light profile is dominated by a smooth, spheroidal component. There is little to no evidence of spiral arm structure or distinct dust lanes. The galaxy exhibits a color gradient, appearing more yellow-orange toward the center, suggesting an older stellar population is dominant in the core. The outer regions are slightly bluer, potentially indicating more recent star formation. There is no obvious major merging activity or tidal disturbances in the image, although minor disturbances cannot be ruled out. The galaxy is moderately luminous and appears to be a relatively massive system.
