The galaxy exhibits a primarily smooth morphology. It appears largely elliptical, with a significant concentration of light towards the central region, suggesting a substantial bulge. The color profile indicates a relatively redder hue, hinting at an older stellar population. There is a subtle disk-like structure, with little indication of strong spiral arms. No major disturbances are evident. There may be some minor disturbances present. Overall, the galaxy presents a mature, possibly quiescent, system.
