The galaxy appears to be a relatively compact object, exhibiting a largely smooth morphology. It is somewhat elongated, though not strongly so. The central region is characterized by a bright, concentrated luminosity, suggesting a significant stellar population and potential activity at the core. The color gradient transitions from a somewhat bluer hue in the central area to slightly redder tones in the outskirts, possibly indicating varying stellar populations and star formation rates across the galaxy. No distinct spiral arms or significant disk features are immediately apparent. There is a subtle suggestion of minor disturbances in the outer regions, but the overall structure appears largely undisturbed.
