The galaxy presents as a relatively small, edge-on spiral, or potentially a lenticular galaxy. It exhibits a smooth, centralized bulge, with a disk that appears elongated, displaying a cigar-like shape. The disk itself shows a mottled texture indicative of some star formation, although it is not pronounced. No distinct spiral arms are apparent. Color gradients suggest a population of older stars dominating the bulge, with bluer regions in the disk potentially tracing younger stellar populations. Overall, the galaxy appears relatively isolated and undisturbed, showing no strong signs of ongoing major merging events, although minor disturbances cannot be ruled out.
