The galaxy presents as a centrally concentrated object with a generally smooth appearance. Its shape is largely elliptical, showing high circularity with a slight deviation from perfect roundness. The galaxy’s color profile exhibits a yellowish-orange hue, possibly indicative of an older stellar population. There is no evidence of prominent spiral arms or a well-defined disk structure. No significant disturbances or tidal features suggestive of ongoing or recent major mergers are discernible. Marginal asymmetries or minor perturbations in the outer regions may hint at past interactions, but the overall morphology suggests a relatively undisturbed system.
