The galaxy presents as an elliptical morphology, with a smooth, relatively featureless structure. It is elongated, appearing to be somewhere between round and cigar-shaped. A concentrated central bulge exhibits a yellowish hue, indicating an older stellar population. The outer regions display a more diffuse profile with a slight bluish tint, potentially suggesting a small amount of ongoing or recent star formation, though at a reduced rate. There is no evidence of significant merging or tidal disturbances.
