The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology with a high degree of roundness in its overall shape. The light distribution appears relatively uniform, lacking any distinct spiral arm features or prominent dust lanes. There is a subtle color gradient, with a slightly yellower core transitioning to a bluer hue in the outer regions. Faint, diffuse emission extends outwards, suggesting a halo component or a gradual decline in stellar density. There is no significant evidence of ongoing mergers or major tidal disturbances in its structure, although some minor asymmetry cannot be entirely ruled out. The galaxy appears to be a relatively isolated system within the observed field.
