The galaxy presents a predominantly smooth morphology, suggestive of an elliptical or lenticular type. The central region exhibits a concentration of light with a yellowish hue, possibly indicating an older stellar population and minimal dust content. Moving outward from the core, the light distribution appears more diffuse and slightly bluer, hinting at the presence of younger stars or a low level of ongoing star formation within a disk-like structure. The overall shape is somewhat elongated, but not extremely so. There is no obvious evidence of spiral arms or significant tidal disturbances, although subtle asymmetries may indicate past or ongoing interactions. The galaxy appears relatively isolated within its immediate surroundings, with no major companions or signs of a major merger event.
