The galaxy presents as an elliptical structure, exhibiting a smooth, largely featureless morphology. The light profile appears centrally concentrated with a gradual falloff in intensity towards the outer edges. It has a moderate ellipticity; the overall shape is more elongated than circular, but not highly flattened. The color index suggests a population dominated by older stars, with a yellowish-orange hue indicative of lower levels of ongoing star formation and a higher proportion of red giant stars. There is no visible evidence of spiral arms, bars, or other distinct structures typically associated with disk galaxies. There does not appear to be a clear disk component.
