The galaxy presents a generally elliptical morphology, exhibiting a smooth, concentrated light distribution. The color profile suggests a dominant older stellar population, with the central region appearing more yellowish-orange, indicative of evolved stars. There is very little evidence of significant dust lanes or spiral arm structure, implying a lack of ongoing, large-scale star formation. The overall symmetry points towards a relaxed system, potentially an evolved galaxy that has undergone significant morphological quenching. Minor disturbances are present, but the galaxy appears to be a largely undisturbed system.
