The galaxy appears as a relatively compact object with a smooth morphology, exhibiting a near-circular shape in projection. Its color profile indicates a dominant population of older stars, based on its redness in optical wavelengths. There is only a slight presence of bluer regions, suggesting either ongoing low-level star formation or the presence of a small population of younger stars. The overall structure shows minimal signs of significant tidal disturbances or recent major merger events. Minor perturbations cannot be excluded with certainty at this resolution.
