The galaxy appears as a relatively smooth, elliptical-like object. It exhibits a generally round morphology, with a slight deviation towards an intermediate shape. There is no clear evidence of prominent spiral arms or a well-defined disk structure. The light distribution appears relatively uniform across the galaxy's body, lacking bright or distinct features indicative of active star formation regions. There are no visible signs of on-going major merging events or significant tidal disturbances affecting the galaxy's overall structure. The galaxy shows a color gradient, appearing somewhat redder in the central regions compared to the outer edges, possibly indicating an older stellar population concentrated towards the center.
