The galaxy presents as a relatively smooth, elliptical structure. Its overall shape is elongated, exhibiting a cigar-like appearance, with a bright, concentrated central bulge. There is a subtle color gradient, with the core tending towards a yellowish-white hue, suggesting a population of older stars. Moving outwards from the core, the galaxy fades into a bluer halo, implying the presence of younger stars and possibly ongoing star formation. No distinct spiral arms or prominent dust lanes are discernible, further supporting its classification as an elliptical galaxy. The outer edges of the galaxy are diffuse, gradually blending into the background sky. There's a slight suggestion of minor disturbances in the outer regions, though they do not appear to constitute a major merger event.
