The galaxy presents a generally smooth, elliptical morphology, appearing largely spheroidal with a high degree of central concentration. Its color profile exhibits a yellowish-orange hue in the core region, suggestive of an older stellar population dominated by red giant stars. The outer regions display a gradual transition to a slightly bluer tint, hinting at the presence of younger, hotter stars in the galaxy's outskirts, potentially indicating recent or ongoing, albeit low-level, star formation activity. There is no clear evidence of spiral arm structure, and the galaxy does not exhibit any significant signs of tidal disturbances or major mergers. Some minor irregularities on the outer edges may indicate interaction with satellite galaxies.
