The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless appearance. The light distribution is concentrated towards the center, forming a bright, yellowish core that suggests a significant population of older stars. Moving outward from the core, the light intensity decreases gradually, fading into a more diffuse halo. The overall shape appears close to circular. There is no discernable spiral structure or evidence of ongoing major mergers or tidal disturbances. The galaxy exhibits colors consistent with a evolved stellar population and suppressed star formation.
