The galaxy appears as a concentrated spheroid of light, with a smooth, largely featureless morphology. The central region exhibits a bright, yellowish-white glow, suggesting a significant population of older stars. A gradual fading in brightness extends outwards from the center, transitioning to a reddish hue in the outer regions. There is no discernable spiral structure or prominent dust lanes. The overall appearance is consistent with that of an elliptical galaxy, showing signs of moderate star formation within its central regions. No signs of any ongoing mergers or major disturbances are visible within the galaxy's morphology. It seems to be a relatively isolated system, without close companions.
