The galaxy presents as a somewhat irregular elliptical structure, exhibiting a centrally concentrated luminosity profile. The core region displays a reddish hue, possibly indicative of an older stellar population or dust obscuration. Surrounding the core is a more extended, greenish halo, which may signify ongoing star formation or the presence of ionized gas. The overall morphology is moderately smooth, with no obvious spiral arms or bar structures visible in this imagery. The galaxy appears to be relatively isolated, lacking any major tidal distortions that would suggest recent or ongoing merger activity, although there are indications of minor disturbances in the galaxy shape. The color gradients suggest varying stellar populations or dust content across the galaxy's structure. The galaxy's estimated size is relatively small, likely a few kiloparsecs across.