The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. The overall color profile indicates a slightly redder hue, suggestive of an older stellar population. The galaxy appears quite round in shape, with only minimal deviation from a perfect circle. No prominent spiral arms, dust lanes, or other distinct features are discernible. There is no strong evidence of any ongoing merging activity or significant tidal disturbances. The galaxy seems to be a single, relatively undisturbed system.