The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge that appears nearly spherical in projection. The color profile suggests an older stellar population, indicated by the yellowish-gold hue concentrated in the core. Fainter, more diffuse, greenish light surrounds the core, potentially indicating regions of ongoing, but low, star formation within the galaxy's disk or halo. Evidence of a developed spiral structure or significant dust lanes are absent; minor irregularities are present, perhaps due to tidal disturbances.
