The galaxy presents as an elongated, lenticular-like structure with a smooth, centrally concentrated luminosity profile. There appears to be minimal evidence of spiral arm structures or prominent dust lanes. The dominant color is reddish-yellow, suggesting an older stellar population with relatively little ongoing star formation. There may be some bluer regions in the disk of the galaxy. The galaxy's shape is somewhat cigar-like. There is no obvious signs of tidal features or morphological distortions suggestive of recent or ongoing major mergers, although a minor interaction cannot be ruled out.
