The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is somewhat elliptical, appearing more 'in between' than perfectly round or cigar-shaped. There is a noticeable central bulge that dominates the light profile. The galaxy exhibits a yellowish-orange hue, suggestive of an older stellar population with minimal ongoing star formation. No prominent spiral arm structures or dust lanes are discernible; the light distribution appears largely uniform, with only subtle variations in color and intensity. There is no obvious evidence of any major merger events, although some minor disturbances or interactions cannot be ruled out.
