The galaxy presents a smooth, elliptical morphology with a high degree of central concentration. There is no discernible disk structure or spiral arm features. The color profile indicates a dominant population of older stars, inferred from the redder hues. The object appears mostly round in shape, with no significant elongation or distortion. No signs of tidal tails or merging features are visible. Overall, the galaxy appears to be a relaxed system consistent with a quiescent evolutionary state, exhibiting characteristics of a spheroidal galaxy.
