The galaxy presents a generally elliptical morphology, though with some apparent irregularities suggesting potential interactions or internal disturbances. The light distribution appears relatively smooth, with a central concentration of luminosity that gradually decreases outwards. There is a noticeable color gradient, with the core region exhibiting a more yellowish/reddish hue, potentially indicative of an older stellar population or significant dust obscuration. Fainter, bluer regions are observed at the periphery, possibly indicating ongoing star formation. The overall orientation shows a slight elongation, and there may be subtle tidal features or distortions present, hinting at past or ongoing gravitational interactions.
