The galaxy presents as a disk galaxy, oriented approximately edge-on from our vantage point. It exhibits a central bulge that appears yellowish-white in color, suggesting a population of older stars. There is evidence of a faint, extended disk component. This disk shows a slight warp, indicative of a possible interaction or past merger event. The spiral arms are tightly wound, though not clearly defined due to the orientation and distance. The color distribution across the disk ranges from yellow-white closer to the bulge, to more bluish hues in the outer regions, suggestive of recent or ongoing star formation in these areas. Overall, the galaxy appears relatively undisturbed. There is no clear indication of a strong tidal interaction or major ongoing merger.
