The galaxy presents a generally elliptical morphology with a smooth appearance. The light distribution is concentrated towards the center, indicating a prominent bulge. There is a slight elongation, but overall, it appears relatively circular. Faint color variations suggest differences in stellar populations or dust content, with the central region exhibiting a yellowish hue and the outer regions showing hints of bluer tones. There is no clear evidence of spiral arms or prominent dust lanes. The galaxy appears relatively isolated and unperturbed, with no obvious signs of recent mergers or tidal interactions.
