The galaxy presents as a moderately luminous, disk-shaped system with an apparent intermediate inclination. The central bulge exhibits a smooth, concentrated appearance with a yellowish-white hue, suggesting a relatively older stellar population. The disk component displays a bluer color, indicative of ongoing star formation. There appears to be some asymmetry in the disk, with one side appearing slightly more extended or disturbed than the other. There is no clearly visible spiral structure, but the disk itself is not perfectly uniform in brightness, possibly due to patchy star formation or dust obscuration. A possible satellite galaxy or tidal feature is seen closer in the lower left. There are no obvious indications of a major merger in progress.
