The galaxy presents as a centrally concentrated, relatively smooth object, approximately round in appearance. The light distribution is generally even across the galaxy, with a noticeable peak in intensity towards the core. The core region exhibits a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually into the background, displaying a bluer tint, which may indicate the presence of younger stars or lower metallicity stellar populations. There is no clear evidence of spiral arms or a distinct disk structure. The morphology suggests an early-type galaxy, likely an elliptical, with no significant signs of recent or ongoing major mergers, although some minor disturbances cannot be ruled out.
