The galaxy presents as an elliptical morphology, appearing relatively smooth and featureless. The light distribution suggests a high degree of central concentration, with a gradual decrease in brightness towards the outer edges. There is a slight elongation, indicating a shape that is more in-between round and cigar shaped, but not a strong disk structure. The overall color is yellowish-orange, potentially indicating an older stellar population and relatively low ongoing star formation. There is no strong evidence of spiral arms, dust lanes, or merging activity. There may be a very slight asymmetry, but the overall appearance is relatively undisturbed.
