The galaxy presents as a relatively smooth, elliptical object. The core exhibits a concentrated, bright, yellowish-orange hue, suggesting an older stellar population. The outer regions show a gradual decrease in luminosity, fading into a bluish halo. There is no clear evidence of distinct spiral arm structure or prominent dust lanes. The overall shape is elongated, with the major axis significantly longer than the minor axis, indicating an elliptical morphology that is not perfectly spherical. There are no signs of strong tidal disturbances or ongoing major mergers, although subtle irregularities in the outer regions could hint at past minor interactions. The object appears largely undisturbed.
