The galaxy presents as an elongated, cigar-shaped structure, suggestive of an edge-on spiral or lenticular morphology. It exhibits a centrally concentrated bulge region, which is slightly orange in color. Fainter blue-ish dust lanes can be seen extending from the central bulge along the galaxy’s length, indicative of cooler star formation regions and dust. The galaxy shows no signs of major mergers, and the overall structure appears relatively undisturbed. There are hints of minor tidal disturbances.
