The galaxy appears as a relatively smooth, elliptical-like structure. It exhibits a concentrated central region. The main body of the galaxy appears to be mostly featureless with a fuzzy halo extending outwards. The colour profile indicates a population of older stars dominating the central bulge, with a slight bluer hue in the outer regions, suggesting some ongoing, but limited, star formation there. There is no clear evidence of a prominent disk or spiral arms. The overall morphology suggests a relatively evolved system, possibly transitioning towards a quiescent state. The lack of significant irregularities suggests that it hasn't experienced a recent major merger event.
