The galaxy presents as a moderately-sized, edge-on disk system. It exhibits a flattened, elongated morphology with a noticeable dust lane obscuring a portion of the central bulge. The bulge appears relatively small and indistinct. The overall color gradient suggests an older stellar population, with a central reddish hue and a subtle bluer tinge towards the outer edges of the disk, potentially indicating recent star formation in these regions. There is evidence of tidal disruption or interaction, with faint, asymmetric extensions or streams visible extending from the main disk, hinting at a possible past merger event or ongoing gravitational interaction with a nearby object.
