The galaxy presents as a centrally concentrated object with a predominantly smooth morphology. There is a noticeable color gradient, transitioning from a warmer, yellower hue at the core to cooler, bluer tones in the outer regions, suggesting differing stellar populations or dust content across the galaxy's radius. The central region appears relatively homogenous. The galaxy's overall shape is largely elliptical, showing a high degree of roundness with only minimal deviations from a perfect circular projection. There is no indication of any major ongoing merger events or significant tidal disturbances. The object's apparent size is relatively small, suggesting it is either intrinsically compact or located at a considerable distance.
