The galaxy presents as a somewhat elongated, elliptical form with a smooth, diffuse light distribution, suggesting a lack of prominent spiral arms or strong disk features. The central region exhibits a higher concentration of light, indicative of a bulge, possibly housing a supermassive black hole. There's a noticeable color gradient from the core outwards, with the central bulge appearing more yellow/orange, potentially indicating an older stellar population compared to the outer regions which appear slightly bluer, suggesting ongoing, albeit low, levels of star formation. There is some evidence of possible minor disturbance or a subtle tidal feature on one side, hinting at a past or ongoing interaction, though no significant merger event is immediately apparent.
