The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that displays a yellowish hue, suggesting an older stellar population. The galaxy appears largely spheroidal. There is a hint of a faint, diffuse halo surrounding the central region, extending outwards. The overall color profile suggests minimal recent star formation. There is no clear evidence of spiral arms or a well-defined disk. The galaxy shows no obvious signs of a major merger event or significant tidal disruption.
