The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual decline in luminosity toward the outer regions. The overall color appears to be relatively red, suggestive of an older stellar population and possibly a lower rate of on-going star formation. There is no apparent dust lane or prominent spiral arm structure. The galaxy appears to be relatively undisturbed, without any signs of major mergers or tidal interactions. The elongated shape suggests that it is not viewed face-on, but rather at an angle relative to our line of sight. Overall, the morphology suggests a relatively evolved system, consistent with an elliptical galaxy type.
