The galaxy exhibits a generally smooth morphology, with some subtle indications of disk-like structure. The overall shape appears somewhat elongated, deviating from a perfectly circular form. There is no strong evidence of ongoing major merging activity or significant tidal disturbances. The light distribution appears centrally concentrated, with a color gradient suggesting a redder core region that may be populated by older stars, with the color of the outer area appearing slightly more blue. The object is faint, but with a distinct central bulge.
