The galaxy presents as a centrally concentrated object, seemingly elliptical in morphology, with a smooth light distribution. The core exhibits a bright, unresolved nucleus, suggesting the presence of an active galactic nucleus or a region of intense star formation. Fainter, more diffuse light extends outwards from the core. The isophotes, though somewhat indistinct, appear generally elliptical, with a moderate degree of ellipticity. There may be a slight color gradient, with the core exhibiting a more blue-white hue and the outer regions having a redder tint, potentially indicating older stellar populations in the outer regions. No obvious signs of spiral arms, bars, or significant dust lanes are discernible in this image. The overall appearance is consistent with an early-type galaxy, with the majority of the object's light concentrated towards the center, suggesting an evolved stellar population. There is no obvious visual disturbance to indicate a recent merger.
