The galaxy presents as a single, luminous object with a smooth and centrally concentrated profile. The core exhibits a yellowish hue, suggesting a population of older stars. Surrounding the core is a diffuse halo, appearing slightly greenish, possibly indicating a small amount of ongoing star formation, or the presence of ionized gas. The overall morphology is fairly regular, and there is no evidence of strong tidal features, merging activity, or significant disk-like structures. The galaxy's roundness indicates a relatively low inclination angle with respect to the line of sight. Based on these characteristics, this galaxy appears to be a relatively massive early-type galaxy, likely an elliptical or lenticular galaxy at a moderate distance.
