The galaxy presents an overall elliptical morphology, appearing largely featureless and smooth in texture. Its color profile suggests a population of older stars, with a yellowish-red central bulge indicative of evolved stellar populations. There are no visible spiral arms or dust lanes. The light is centrally concentrated, diminishing gradually toward the outer edges, suggesting minimal on-going star formation. There is no evidence of a strong tidal interaction, though a slight asymmetry in the outer halo region might suggest minor past interactions. The galaxy does not appear to be actively merging.
