The galaxy presents as a relatively smooth, elliptical morphology. The core is noticeably brighter and more concentrated compared to the outer regions. The overall color appears to be yellowish-orange, suggestive of an older stellar population. There is minimal evidence of spiral arm structure or significant dust lanes, although there are some very faint wisps or features that could potentially be tidal debris. The galaxy is somewhat elongated, appearing somewhere in between a circular and cigar shape. There is no obvious signs of a major merger, or any major disturbances in its shape.
