The galaxy presents as a spiral galaxy, viewed nearly edge-on. The galactic disk appears as a flattened, elongated structure, with a bright central bulge. The bulge exhibits a smooth, rounded morphology, suggesting a relatively old stellar population.

The disk displays an uneven distribution of light, with some regions appearing more luminous than others. Evidence of dust lanes is subtle but potentially present, obscuring the light from stars within the disk. The galaxy appears reddish in color, hinting at the presence of older stars and dust. There's no obvious indication of intense star formation activity, like strong emission nebula. There appears to be no major ongoing merging event, however there may be some minor gravitational disturbances occurring in the disk.
