The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central region. The color profile indicates a predominantly older stellar population, evidenced by the yellowish-orange hue. There is little to no evidence of distinct spiral arms or prominent dust lanes. The overall morphology suggests a system where star formation is currently suppressed, possibly due to the galaxy's advanced age or environmental effects. There is potentially minor gravitational disturbance occurring, but it's difficult to tell given the images characteristics. The shape of the galaxy is somewhere in between a perfect circle and an ellipse. 