This galaxy exhibits a roughly elliptical morphology. Its core is bright and concentrated, with a yellow-white hue, suggesting an older stellar population. Extending outward from the core, there is a fainter, more diffuse halo with subtle extensions, possibly tidal features. The color of this halo appears slightly bluer than the core, which might indicate the presence of younger stars or recent star formation in the outer regions. There is evidence of disturbances in the structure. Faint wisps and asymmetries suggest a past interaction or a possible minor merger. Although it appears mostly smooth, subtle variations in surface brightness suggest underlying structures such as faint spiral arms or shells. Overall, this galaxy presents an interesting mix of smooth features and potential dynamical disturbances.