The galaxy presents as a largely elliptical structure with a smooth, diffuse light distribution, suggesting a relatively evolved system. There is minimal evidence of spiral arms or a defined disk component. The galaxy's light profile appears moderately concentrated towards the center, hinting at a substantial galactic bulge. No significant tidal features or morphological disturbances are immediately apparent, indicating that the galaxy is likely not undergoing a major merger event. There may be some slight irregular features, suggesting possible minor interactions. The galaxy displays a color gradient, appearing bluer in the outer regions and redder towards the core.
