The galaxy presents as an elliptical system, exhibiting a generally smooth and rounded morphology. Its core region appears concentrated and luminous, transitioning gradually outwards to a less defined, diffuse halo. The color profile suggests a dominant population of older stars, implying a low star formation rate. No prominent spiral arms, dust lanes, or other distinct features are apparent, which supports a classification of the system as an early-type galaxy. There is no indication of any ongoing major merger activity. The shape is close to round.
