The galaxy appears to be a relatively smooth, elliptical-type system. It exhibits a concentrated central bulge with a diffuse, extended halo. The color profile suggests a population of older stars, with a slightly redder hue dominant in the central regions, implying a lack of significant recent star formation. The galaxy displays a generally rounded morphology, with no obvious signs of spiral arms or a distinct disk structure. There might be minor gravitational disturbance, but the overall shape is well-defined.
