The galaxy appears as a centrally concentrated object with a smooth, slightly elliptical morphology. The core region exhibits a high surface brightness, indicative of a dense stellar population or active galactic nucleus. The color profile suggests the presence of younger, bluer stars predominantly within the central region, possibly indicating ongoing or recent star formation.  The galaxy lacks prominent spiral arms or a distinct disk structure. There is a subtle asymmetry in the outer halo, hinting at possible past interactions or minor disturbances affecting its structure. Overall, the galaxy appears relatively isolated with no obvious signs of a major merger event.
