The galaxy exhibits a generally elliptical morphology, appearing relatively smooth in structure. A pronounced central bulge is evident, characterized by a concentrated, bright yellowish-white glow, suggesting a high density of older stellar populations. The outer regions of the galaxy gradually fade into a more diffuse halo, showing a transition in color towards a slightly bluer hue. This color variation could indicate the presence of some younger, bluer stars in the galaxy's outskirts, although the overall stellar population seems to be dominated by older stars. There appears to be very little dust present, which may contribute to the overall smooth and featureless appearance. There is no obvious spiral arm structure or significant tidal disturbances indicating a possible merger event, though there is a slight distortion in shape. The galaxy appears generally isolated and does not show any signs of interaction with nearby galaxies.
