The galaxy presents as a generally smooth, elliptical-like form. The central bulge appears bright and concentrated, exhibiting a yellowish-white hue, indicative of an older stellar population. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape. Fainter, diffuse extensions surround the brighter central region, gradually fading into the background sky. These extensions lack distinct spiral arm structures or prominent dust lanes. There are possible hints of disturbed features suggesting the potential of recent or ongoing interactions. The overall color profile suggests that star formation is suppressed. 
