The galaxy presents as a relatively smooth, elliptical object with a concentrated central bulge. Its overall form appears well-defined and largely undisturbed. The color gradient exhibits a yellowish hue, transitioning to slightly redder tones in the outer regions, suggestive of an aging stellar population. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's morphology indicates a system dominated by evolved stars and potentially low current star formation. A lack of significant tidal features suggests it has not undergone a major merger recently. The overall appearance is consistent with a galaxy at intermediate redshift, where the intrinsic luminosity allows for detailed study despite its distance.
