The galaxy presents as a centrally concentrated object with a generally smooth morphology. The overall shape approximates a flattened spheroid, appearing more rounded than elongated, with a slight ellipticity noticeable in the overall form. The light distribution is heavily concentrated towards the core, with a gradual fading of luminosity towards the outer regions. A subtle color gradient appears to be present, transitioning from a bluer hue in the central region to a slightly redder hue in the outer regions. There is no definitive evidence of prominent spiral arm structures or a distinct disk component. There are no signs of major mergers or significant tidal disturbances affecting the main body of the galaxy, though very subtle irregularities may indicate some minor gravitational interaction. The general form implies a system that is relatively undisturbed and quiescent in terms of major mergers or active starburst activity.
