The galaxy presents as a slightly elongated, lenticular or early-type spiral. It exhibits a generally smooth appearance with a concentrated central bulge that graduates outward into a less defined disk. Color gradients suggest an older stellar population dominates, with yellowish hues concentrated in the central regions, indicating a likely lack of significant recent star formation. Hints of blue suggest areas of more recent stellar formation. Faint disturbances or asymmetries are noticeable. Based on morphological analysis, the galaxy is likely not undergoing any major mergers, exhibiting a smooth, centralized structure. The size and shape of the galaxy suggests it's a normal sized galaxy.
