The galaxy presents a largely smooth, elliptical morphology. It is characterized by a concentrated central bulge, exhibiting a yellowish-orange hue, suggesting an older stellar population. The overall form appears quite rounded, with minimal deviation from a circular shape. A subtle halo of bluish light surrounds the central region, possibly indicative of a younger stellar population. There is no evidence of distinct spiral arms or a prominent disk structure. The galaxy appears relatively undisturbed, with no obvious signs of ongoing or recent major mergers, although there are hints of minor disturbances. Overall, the galaxy appears to be a relatively massive early-type galaxy with a moderate level of star formation.
