The galaxy exhibits a generally elliptical morphology, appearing as a smooth, centrally concentrated object. The color gradient transitions from a yellowish core to a slightly bluer, diffuse outer region. There is no apparent spiral structure or distinct dust lanes visible. The galaxy appears relatively isolated, with no obvious signs of tidal interactions or ongoing mergers, although there is a slight asymmetry to the outer halo. There might be a hint of faint, extended structure in the periphery, but this is difficult to resolve with certainty at this resolution. The overall impression is of a mature galaxy with a fairly quiescent star formation rate.
