The galaxy presents a largely smooth morphology, suggestive of an elliptical galaxy. It exhibits a generally round shape, with a slight deviation from perfect circularity. The galaxy's color profile indicates a higher concentration of older stars, given the predominantly reddish-yellow hue in the central region. There is minimal evidence of ongoing star formation, which is consistent with the galaxy’s color. The image shows no signs of spiral arms or a prominent disk structure. There are no indications of any major mergers or significant tidal disturbances, although a very slight asymmetry could suggest a minor past interaction. Overall, the galaxy appears to be a fairly evolved system, mostly comprised of an older stellar population with a relatively high mass.
