The galaxy exhibits a largely smooth, elliptical morphology, characterized by a centrally concentrated light distribution. The core region displays a yellowish-white hue, indicative of an older stellar population. Moving outward from the core, the color gradient transitions towards a slightly bluer shade, though the overall color remains relatively red. There is no apparent spiral arm structure or prominent dust lanes visible. The galaxy appears relatively undisturbed, showing no strong evidence of ongoing major merger activity or tidal distortions. A slight asymmetry is observed in the outer regions, but it is not a prominent feature. The effective radius is estimated to be a few kiloparsecs, classifying it as a medium sized galaxy. The observed color profile suggests a low star formation rate.
