This galaxy appears to be a relatively smooth, centrally concentrated object, exhibiting a somewhat elliptical morphology. There is a noticeable color gradient, shifting from a redder core region to a bluer halo. The galaxy does not present any prominent spiral arms, bars, or other features indicative of significant disk structure. Faint signs of disturbance seem to be present, though they are not distinct enough to be considered a major merger. The overall light distribution suggests an older stellar population, particularly towards the core, while the surrounding areas seem to contain pockets of more recent, though currently limited, star formation.
