This galaxy exhibits a generally smooth morphology, suggesting an elliptical or lenticular classification. The central region presents a concentrated, bright core, fading outward to a more diffuse halo. The overall shape is somewhat rounded, though not perfectly spherical. There is subtle evidence of faint, extended features, but no significant spiral arm structure or bar is discernible. The color profile indicates a population of older stars, with the core appearing more yellow/white, indicative of less active star formation. Areas of reddish hue are sparsely distributed, possibly indicating regions of dust or older stellar populations. There does not appear to be evidence of ongoing major merger activity, though minor tidal disturbances cannot be ruled out. The galaxy's moderately compact size suggests it is a relatively quiescent system.
