The galaxy presents as a somewhat elliptical structure, displaying a smooth, diffuse light distribution. A prominent central bulge is evident, exhibiting a yellowish hue, which may indicate an older stellar population. Fainter, bluer regions are observed extending outwards from the central bulge along the major axis, possibly indicating the presence of younger stars or ongoing star formation. The disk appears relatively featureless, with little evidence of distinct spiral arms or dust lanes. The galaxy shows some visual elongation, with a ratio of major to minor axis suggesting an intermediate inclination angle.
