The galaxy presents as an elliptical, spheroid-dominated system. It appears smooth in texture with no discernible spiral arms or significant dust lanes. The color distribution indicates a higher concentration of older stellar populations, based on the concentration of redder colors in the central bulge. There is an elliptical halo of blue-ish light surrounding the redder core, indicating some younger stars may be present. The galaxy exhibits a cigar-like shape in its overall morphology, with its major axis being more than twice the length of its minor axis. There is no evidence of any major merging activity or strong tidal disturbances affecting the structure of the galaxy. Faint asymmetric features are suggested, indicating possible minor disturbances.
