This galaxy presents as a largely featureless elliptical, with a high degree of central concentration. The light distribution appears smooth and centrally condensed, indicative of an older stellar population. There is a subtle color gradient from the center outwards, with the core exhibiting a yellowish-white hue, potentially indicating a higher concentration of evolved stars. The outer regions are fainter and have a slightly bluer tint, possibly due to a small amount of residual star formation. There is no evidence of spiral arms, a bar structure, or any major tidal disturbances in this image. Overall, the galaxy appears to be a relatively isolated system in a late stage of its evolution.
