The galaxy presents a largely smooth morphology, with minimal visible features suggestive of spiral arms or a prominent disk structure. The light distribution appears centrally concentrated, exhibiting a high degree of radial symmetry. The shape is approximately elliptical, with a slight deviation towards a more oblate form, but it is mostly round. There is no evidence of ongoing major merging activity or significant tidal disturbances. The color profile suggests a dominance of older stellar populations, reflected in the redder hues observed in the outer regions. A bluer core could indicate some residual star formation, but the overall star formation rate appears quite low. The galaxy shows a significant degree of structural homogeneity.
