The galaxy presents as a largely smooth, elliptical-like structure. Its core exhibits a high degree of central concentration, gradually fading towards the outer edges. While seemingly undisturbed, a very slight asymmetry or distortion can be observed in the outer halo, indicating a potential, albeit minor, interaction or tidal disturbance. The overall color appears to be trending towards the redder end of the spectrum, consistent with a relatively older stellar population and a lower ongoing star formation rate. The shape of the galaxy appears to be more "in-between" round and cigar shaped. It does not appear to be undergoing a major merger.
