The galaxy presents as a diffuse, ellipsoidal structure with a distinct radial color gradient. The core region exhibits a reddish hue, suggestive of an older stellar population and/or dust obscuration. Progressing outwards, the color shifts towards a greenish-blue, hinting at the presence of younger, hotter stars and possibly ongoing star formation activity in the galaxy's periphery. No defined spiral arms or bar structures are discernible, and the overall morphology appears relatively smooth. The galaxy shows no obvious signs of major mergers or significant tidal disturbances.
