The galaxy presents as a roughly elliptical, diffuse structure with a smooth, relatively featureless morphology. The overall color appears slightly redder, suggestive of a population dominated by older stars, potentially indicating a relatively low star formation rate. There is a slight elongation observed, with a relatively round morphology. There might be a faint suggestion of a minor interaction or disturbance on one edge, though it is difficult to say for certain. The central region of the galaxy appears slightly more concentrated in luminosity than the outer regions. Overall, the galaxy appears relatively undisturbed and evolved.
