The galaxy presents as a flattened, disk-shaped system, observed at a near edge-on inclination. A prominent central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. The disk component displays a bluer color, indicating the presence of younger stars and ongoing star formation. Faint, patchy structures extending outward from the central region hint at spiral arm features, though these are not clearly defined due to the inclination and moderate distance. There is no obvious evidence of major mergers or significant tidal disturbances in the immediate vicinity of the galaxy, though minor asymmetries in the outer disk regions may suggest some past interaction. The overall structure suggests a disk galaxy, likely a spiral, with moderate star formation activity.
