The galaxy presents as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge that fades gradually into a more diffuse halo. There are no distinct spiral arms visible. The galaxy appears to be relatively round. Based on color, stellar populations are likely older, with lower rates of recent star formation, resulting in a redder overall hue. There is no evidence of significant tidal disturbances or ongoing mergers, based on the lack of lopsidedness or disrupted morphology.
