The galaxy presents as a slightly elongated, disk-shaped object with a concentrated central bulge. The bulge exhibits a yellowish-white hue, indicative of an older stellar population. Surrounding the bulge is a bluish disk, suggesting the presence of younger, hotter stars and ongoing star formation. The disk appears relatively smooth with only subtle variations in brightness. The galaxy is tilted with respect to the observer's line of sight. There is evidence of some minor disturbance or interaction affecting the galaxy’s morphology. The overall light distribution indicates a centrally concentrated profile.
