The galaxy presents as a relatively smooth, elliptical-like structure with an apparent red shift, indicating a considerable distance. It appears to be moderately massive, exhibiting a central bulge that dominates the light profile. A faint disk is present and is viewed at an angle. The disk exhibits a bluer color profile, indicative of ongoing star formation, and is surrounded by a smooth, diffuse halo of relatively older stars. The morphology suggests a moderate rate of star formation. There's no prominent evidence of major mergers or significant tidal disturbances, though a slight asymmetry in the outer regions could hint at minor interactions.