The galaxy presents as a relatively smooth object, suggestive of an elliptical or lenticular morphology. Its overall color profile indicates a predominantly older stellar population, with a yellowish-orange hue dominating the central bulge region. There is minimal evidence of spiral arm structure or significant dust lanes, reinforcing the smooth classification. The ellipticity of the galaxy indicates a deviation from perfect circularity, with the major axis appearing significantly longer than the minor axis, suggesting a slightly elongated shape. There may be minor disturbances present within the extended halo. There is no noticeable merging activity apparent from its morphology.
