The galaxy presents an elliptical morphology, exhibiting a smooth, featureless appearance in optical wavelengths. Its color profile suggests a relatively older stellar population, with a noticeable concentration of light toward the galactic center, indicative of a bulge. While a disk component cannot be entirely ruled out based on this image, its prominence appears minimal. There is no evidence of ongoing major mergers or significant tidal disturbances, although a subtle asymmetry might suggest minor past interactions. The galaxy appears relatively isolated in its immediate environment. Overall, this is likely a passively evolving elliptical galaxy.
