The galaxy presents a smooth, elliptical-like morphology. Its light distribution is dominated by a central bulge, with a high degree of concentration. The galaxy appears to be mostly featureless, lacking prominent spiral arms or dust lanes. There is some evidence of possible tidal disturbance or minor merger activity. Overall, the galaxy appears relatively evolved, with a redder color indicative of an older stellar population. The galaxy shows a moderate star formation rate and has a considerable stellar mass. 
