The galaxy presents as a somewhat diffuse, elliptical structure with a dominant central bulge. The light distribution appears relatively smooth, with a subtle color gradient from a yellowish-white core to slightly bluer outer regions. No distinct spiral arm features are visible, nor is there any indication of a well-defined disk structure. The overall shape is neither perfectly round nor significantly elongated, with a moderate axis ratio. Some subtle asymmetries or minor disturbances seem to be present, possibly indicating ongoing or past interactions. There appears to be no strong evidence of a major merger or tidal tails, however, some faint light might extend beyond the main body of the galaxy.