The galaxy presents as an elliptical or lenticular morphology, with a smooth, centrally concentrated luminosity profile. The core region exhibits a bright, yellowish hue, indicative of an older stellar population. Moving outward from the center, the color becomes slightly bluer, suggesting a minor presence of younger stars in the outer regions. The overall shape is moderately elongated, appearing more cigar-shaped than circular. There is no strong evidence of spiral arms or a distinct disk structure. Furthermore, there are some hints of minor disturbances in the outer regions, but overall the galaxy appears relatively undisturbed.
