The galaxy presents a generally smooth morphology, appearing largely featureless in this imaging. It exhibits a radial symmetry, tending towards a circular shape when viewed in projection. There is little to no evidence of spiral arms or a defined disk structure; rather the light is distributed evenly. Faint color variations can be observed, with a subtle shift towards redder hues in the central regions, suggesting an older stellar population. No apparent signs of mergers or significant tidal disturbances are noticeable, further supporting the galaxy's classification as relatively undisturbed. Overall, the galaxy appears as a single, well-defined object.
