The galaxy presents as a concentrated spheroid of light, largely featureless in its central region. The overall color appears to be a slightly reddish-yellow hue. There is little evidence of distinct spiral arm structures or prominent dust lanes, suggesting a relatively smooth morphology. The concentration of light is highest at the galaxy's core, with a gradual decrease in intensity towards the outer edges. There appears to be some mild asymmetry and potentially a slight distortion in the outer regions, which could indicate past or ongoing minor gravitational interactions with smaller satellite galaxies. Its light indicates a significant amount of older stellar populations. The overall impression is that of a massive galaxy, relatively evolved, and potentially undergoing or having undergone some mild disruption.
