The galaxy presents a generally smooth, elliptical morphology, appearing nearly round on the plane of observation. Its light profile suggests a fairly concentrated core with a gradual decrease in intensity towards the outer regions, lacking well-defined spiral arm structures. The galaxy exhibits a reddish-yellow hue overall, indicative of an older stellar population and possibly a lower rate of current star formation. Subtle irregularities in the outer regions hint at minor gravitational interactions or past merger events, although the overall structure is largely undisturbed. The galaxy demonstrates a notable size and a significant luminosity, indicating a substantial stellar mass.
