The galaxy presents a relatively smooth morphology, appearing elliptical in shape. It exhibits a distinct central bulge characterized by a yellowish hue, potentially indicative of an older stellar population. Moving outward from the core, a gradual transition to a more elongated structure is observed, with hints of a disk-like component. The overall color gradient suggests a radial variation in stellar populations and/or dust content, with bluer regions possibly indicating areas of more recent star formation. There is no immediately visible evidence of strong tidal disturbances or ongoing major mergers, although subtle asymmetries might indicate minor past interactions. The galaxy appears reasonably isolated, with no immediately apparent companion galaxies in close proximity.
