The galaxy presents as a highly inclined, nearly edge-on disk galaxy. A prominent central bulge dominates the light profile. The bulge appears smoothly distributed with a slight elongation parallel to the disk. The disk itself is thin and elongated, with the highest concentration of light towards the mid-plane. The color gradient indicates a redder hue, which implies a population dominated by older stars and a reduced rate of on-going star formation. No clear dust lanes or spiral arm structures are visible in this image, which may be due to the high inclination or to the overall characteristics of the galaxy. There is no apparent evidence of a major merger or significant tidal disruption. Faint asymmetric features suggest some minor gravitational interaction could be taking place.
