The galaxy presents as a somewhat smooth, elliptical-like structure. It has a noticeable elongated shape, appearing more cigar-shaped than perfectly round. The central region exhibits a concentrated brightness, suggesting a significant stellar density or perhaps an active galactic nucleus. The overall color profile appears to be on the redder side, which could indicate an older stellar population and a lower rate of ongoing star formation. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears relatively isolated with no obvious signs of major mergers or tidal disturbances.
