The galaxy presents as an elliptical morphology, exhibiting a smooth, featureless appearance. Its shape is roughly intermediate between round and elongated, tending toward round. The galaxy's light profile is concentrated towards the center, displaying a bright yellowish-white core that gradually fades into the surrounding halo. There is no visible evidence of spiral arms, bars, or significant dust lanes. The overall color suggests a relatively older stellar population, consistent with a low ongoing star formation rate. No apparent signs of major mergers or significant tidal disturbances are observed in the immediate vicinity, though a minor disturbance cannot be ruled out.
