The galaxy presents as a lenticular or early-type spiral galaxy, viewed at a significant angle, close to edge-on. It exhibits a smooth, elliptical profile with a bright, concentrated central bulge that appears yellowish-orange in color, suggestive of an older stellar population. The disk is faint, showing little evidence of distinct spiral arm structure or prominent dust lanes. The disk seems elongated, indicating the edge-on view. The color gradient suggests that the galaxy consists of primarily older stars, indicating a relatively low star formation rate. There is no evidence of a recent major merger event, although the lack of well-defined features hinders a thorough assessment of tidal disturbances.
