The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears elliptical to slightly lenticular, displaying a moderate degree of roundness. A subtle color gradient is observed, with the central region exhibiting a somewhat bluer hue compared to the outer regions, which appear more red. There might be a very slight indication of a disturbance in the galaxy's shape, possibly suggesting a minor interaction or past merger event. No distinct spiral arms or well-defined disk structure are readily apparent. Overall, the galaxy appears to be a mature system with a moderate level of star formation activity.
