The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated light profile with a gradual decrease in luminosity towards the outer regions. The core appears bright and slightly yellowish-white, indicative of an older stellar population. There is very little evidence of spiral arm structure or distinct dust lanes. The overall shape is generally round, with only a slight deviation toward a cigar shape. There is no obvious sign of any ongoing merging activity or major disturbances in the morphology. There may be a very faint, diffuse halo surrounding the central body of the galaxy, extending slightly beyond the main concentration of light. Overall, the galaxy appears to be a relatively undisturbed and mature system.
