The galaxy presents a relatively smooth morphology, appearing elliptical in shape rather than displaying prominent spiral arms or a distinct disk structure. The central region exhibits a high concentration of light, suggesting a substantial bulge component. Moving outward from the center, the luminosity gradually decreases, indicating a diffuse halo. The galaxy displays a generally round profile, with only a slight deviation toward an elongated shape. Some minor disturbances or irregularities in the outer regions hint at possible interactions or past mergers, but overall, the galaxy appears relatively undisturbed. The color gradient suggests a potentially older stellar population dominating the bulge, with the outer regions possibly containing bluer, younger stars, implying ongoing star formation, even if at a moderate level. The estimated size of the galaxy is in the range of a small to intermediate-sized galaxy.
