The galaxy presents a somewhat irregular morphology, exhibiting characteristics of both smooth and possibly disturbed features. A dominant central bulge region displays a smoother texture, with a concentration of older stars giving a yellowish hue. Surrounding the core, a fainter, more diffuse region appears to hint at a faint, disk-like structure, possibly containing areas of active star formation as suggested by a slight bluish tint. The overall shape is largely rounded, but there might be signs of minor gravitational interactions or internal disturbances, observable as a slight asymmetry in the outer regions. It's likely a relatively massive system, and shows moderate star formation activity. There is a possibility that a portion of light is obscured by dust. Overall, this galaxy seems to be in a state of transition or interaction, with a combination of evolved stellar populations and ongoing star formation.
