The galaxy presents as an edge-on or nearly edge-on disk galaxy. A prominent central bulge dominates the morphology, appearing smooth and somewhat spheroidal. The bulge exhibits a concentrated brightness, suggestive of a high stellar density. The disk component is thin and relatively faint, with a noticeable dust lane obscuring portions of the light from the far side. There appears to be minimal evidence of spiral arm structure. The galaxy presents a redder color in the central bulge. The color and morphology suggest that the galaxy has a relatively low rate of active star formation and is likely populated by an older stellar population. There is no significant evidence of tidal interactions or recent merger activity.
