The galaxy presents as an elliptical-like structure with a concentrated, bright core. A somewhat smooth light distribution surrounds this core, extending outward in a diffuse manner. The galaxy displays a slight elongation, appearing more oval than perfectly circular. There is a subtle color gradient noticeable, with the central regions trending towards warmer hues, suggesting an older stellar population, while the outer regions exhibit a slightly cooler tone. No distinct spiral arm features or significant dust lanes are discernible. There is a slight suggestion of a subtle disturbance in the overall structure.
