The galaxy presents as an elliptical morphology, exhibiting a generally smooth, concentrated light distribution without discernible spiral arms or a well-defined disk structure. The galaxy's color profile suggests a population dominated by older stars, evident in the redder hues. The galaxy displays a roughly spherical appearance. There is no apparent evidence of ongoing major mergers or significant tidal disturbances. The star formation rate is estimated to be low. The galaxy's high mass indicates a large stellar population.
