The galaxy presents as a relatively compact and luminous object. Its morphology appears largely elliptical, with a high degree of central concentration. The light distribution is smooth and lacks any distinct spiral arms or prominent features characteristic of disk galaxies. There is a subtle elongation to the shape, departing slightly from perfect sphericity. No significant tidal disturbances or signs of ongoing major mergers are readily apparent, although some minor asymmetry might suggest past interactions. The overall color suggests a population dominated by older stars, consistent with a low ongoing star formation rate. The galaxy's size appears moderate, occupying a small region of the field.
