The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits high luminosity, appearing almost uniformly bright with a slightly yellowish hue. A gradual decrease in surface brightness extends outwards from the core. There appears to be some subtle asymmetry in the outer isophotes, suggesting a possible minor disturbance or interaction in its past. There is no clear evidence of spiral arm structures or significant dust lanes. The overall color profile indicates a population of older stars with relatively low levels of ongoing star formation.
