The galaxy appears to be an elliptical galaxy with a relatively smooth, featureless structure. It exhibits a concentrated central bulge that transitions into a diffuse halo. The light profile appears centrally concentrated, with brightness decreasing gradually outward. The overall shape is slightly elongated, deviating from a perfectly circular morphology. There is a slight hint of a disk-like structure, but that may be due to the angle that we observe it at. The galaxy shows little evidence of active star formation. Overall, the galaxy appears to be a relatively evolved system, consistent with an older stellar population. There is no clear signs of ongoing merger events or tidal disturbances. The galaxy has a reddish hue due to the higher number of older stars.
