The galaxy presents a moderately elliptical morphology, appearing more elongated than circular. A bright, concentrated central bulge dominates the galaxy's luminosity. The outer regions show a diffuse, disk-like structure with a faint spiral arm pattern discernible. The color gradient suggests an older stellar population, exhibiting a yellowish hue throughout the main body. A small region of bluer light indicates some recent star formation. There is an indication of a possible minor interaction or disturbance in the morphology. Overall, it appears to be a relatively massive galaxy with a moderate amount of ongoing star formation.
