The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a concentrated, bright yellowish-white luminosity, suggestive of a population of older, evolved stars. There is a gradual decrease in luminosity moving outward from the core, with the outer regions displaying a fainter, somewhat diffuse halo. The galaxy lacks any obvious spiral arm structure or significant dust lanes. The overall shape appears nearly round, with only a slight deviation from perfect circularity. There is no clear evidence of ongoing merging activity or major tidal disturbances, though minor irregularities cannot be ruled out at this resolution. The galaxy exhibits a red color index. Overall, it appears to be a relatively quiescent, massive galaxy.
