The galaxy presents as a single, relatively smooth object with a concentrated central region. The overall shape is elliptical, appearing mostly round but with a slight elongation to one side. The light distribution suggests a bulge-dominated morphology with a gradual fade towards the outer regions.

There are no apparent spiral arms or prominent dust lanes visible. The color gradient indicates a possible change in stellar population from the core to the outskirts, with the central region showing a yellowish hue, possibly indicative of older stellar populations or dust obscuration. The outer regions appear slightly bluer, perhaps suggesting the presence of younger stars, though this is subtle. There are no clear signs of ongoing major merging events. Some minor disturbance or tidal features cannot be ruled out. The galaxy exhibits a red shift suggesting it is at an intermediate distance.
