This galaxy presents as a relatively smooth, elliptical-like structure. It is centrally condensed, exhibiting a bright core region that gradually fades into a diffuse halo. The overall shape approximates a round form, showing minimal deviation towards a cigar-like morphology. There is no clear evidence of spiral arms or significant disk structures. Faint, potentially disturbed, features or tidal tails are not apparent in the image. No evidence of ongoing major merger events is present, though the possibility of minor disturbances cannot be ruled out based on this image alone. The galaxy appears to be a mature system.
