The galaxy presents as a relatively small, elongated structure, visually classified as a possible edge-on spiral or a lenticular galaxy. Its central bulge appears prominent and exhibits a yellowish-white hue, suggestive of an older stellar population. A faint disk is observed extending from the bulge, appearing somewhat thin and cigar-shaped. There is a noticeable redder region near one end of the disk, potentially indicating areas of dust obscuration or localized star formation. The overall smoothness of the galaxy suggests a relatively quiescent system, possibly with low levels of ongoing star formation. There is no obvious evidence of strong tidal interactions or a recent major merger event.
