This galaxy exhibits a primarily elliptical morphology, but also some possible disk-like or merging features. The central region is characterized by a concentrated area of older stars, presenting a smooth, yellowish-orange appearance. A suggestion of a disk-like component or a merging feature with signs of more active star formation, appears as a faint greenish-blue tint, potentially indicating the presence of younger, hotter stellar populations. The galaxy's overall structure shows some signs of tidal disturbances or interaction with another galaxy, as indicated by the diffuse and somewhat irregular outer regions. Some patches are more concentrated than others, leading me to think it is an active star-forming galaxy.
