The galaxy presents an elongated, cigar-shaped morphology. The light distribution is relatively smooth, with a concentration towards the central region, suggesting a possible bulge. The overall color is yellowish-orange, possibly indicating an older stellar population or significant dust content, consistent with a low star formation rate. There are subtle hints of asymmetry or tidal features, potentially suggestive of past interactions or minor disturbances, but these are not dramatically disruptive to the galaxy's overall structure. The lack of distinct spiral arms or prominent blue regions supports the idea that this galaxy has a relatively low specific star formation rate.
