The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge with a diffuse halo extending outwards. The color profile suggests an older stellar population, with a yellowish-red hue dominating. There is little evidence of spiral arms or dust lanes. The galaxy appears relatively isolated with no obvious signs of interaction or recent merger events, although some minor asymmetries could indicate a previous interaction. Its elongated shape suggests a possible transition from an elliptical to a more lenticular form. The star formation rate appears relatively low, indicative of a quiescent galaxy nearing the red sequence.
