The galaxy exhibits an elliptical morphology, appearing mostly smooth in structure. Its light profile is centrally concentrated with a gradual decline in surface brightness outward, suggestive of an older stellar population dominating the core. There is a slight asymmetry or extension visible, hinting at possible past interactions or internal dynamics influencing its shape. The color profile indicates a redder hue in the central regions, transitioning to slightly bluer tones in the outskirts. This color variation could imply ongoing, though possibly subdued, star formation in the outer regions or differences in stellar populations and dust content. The galaxy appears relatively isolated, with no immediately obvious signs of major mergers or significant tidal disturbances in this image.
