The galaxy appears as a relatively smooth, elliptical object. It exhibits a concentrated central bulge that fades into a more diffuse halo. The color profile suggests a generally older stellar population, with a yellowish hue dominating the central region, indicative of evolved stars. There is little evidence of distinct spiral arms or significant dust lanes. The galaxy's overall morphology points towards a system that has largely exhausted its gas supply and star formation activity. No major disturbances or merging activity is apparent from its general structure, though the light has likely been redshifted due to its distance.
