The galaxy presents a predominantly smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish-orange in color, suggesting an older stellar population. The outer regions of the galaxy display a fainter, more diffuse halo with subtle hints of a bluish-green hue, which might indicate the presence of younger, hotter stars or ongoing star formation, although this is not readily apparent. There is very little evidence of defined spiral arms or significant dust lanes. The overall structure appears relatively undisturbed, with no obvious signs of a major ongoing merger, although there is a slight asymmetry in the halo, possibly indicating a minor interaction or internal dynamics. The galaxy is moderately bright and reasonably well-defined, indicating a substantial mass.
