The galaxy appears to be a relatively smooth, centrally concentrated system. Its morphology suggests a possible elliptical classification, exhibiting a predominantly spheroidal shape with little indication of spiral arms or a well-defined disk structure. The light distribution gradually decreases from the core to the outer regions, indicating a high degree of symmetry. There is a slight elongation observed, though it is not significantly cigar-shaped. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions, though subtle indications of minor interactions can't be fully ruled out. The color gradient shows a central reddish hue that fades toward the edges. The relatively red color suggests a more evolved stellar population in the core, while the bluer outer regions may indicate ongoing star formation. Overall, the galaxy is consistent with being a relatively massive system exhibiting moderate star formation.
