The galaxy presents a generally smooth, elliptical morphology. The light distribution exhibits a concentration towards the center, suggesting a prominent bulge. The overall color appears yellowish-white, possibly indicating an older stellar population dominating the light output. Some subtle bluer regions are visible in the outer parts of the galaxy, which could be indicative of areas with more recent star formation, though they do not appear very prominent. The galaxy appears somewhat elongated, possibly cigar-shaped. There is no visually clear evidence of a spiral arm structure or any ongoing major merger activity. The overall impression is that of a relatively undisturbed, evolved system.
