The galaxy appears as a centrally concentrated, ellipsoidal object. Its color profile suggests an older stellar population, with reddish hues dominating the central regions. The galaxy exhibits a generally smooth texture, with minimal signs of internal structures such as spiral arms or a prominent disk. There is a slight irregularity in its outer isophotes, possibly indicating minor gravitational interactions or recent accretion events. The galaxy has a relatively compact size and a moderate degree of roundness. The overall morphology suggests that this is likely a galaxy in the process of or having already undergone significant stellar evolution, shifting its composition and features.
