The galaxy appears to be an elliptical galaxy, exhibiting a smooth, rounded morphology. There are no readily apparent spiral arms or a significant disk component. The light distribution is concentrated towards the center, suggesting a dominant bulge. The galaxy has a slight color gradient, transitioning from a brighter, whiter core to a dimmer, more reddish-yellow halo. The core's color suggests the presence of a population of hot, young stars or an active galactic nucleus, while the halo's color could indicate an older stellar population. No signs of any major mergers or tidal disturbances are observed.
