The galaxy appears to be a smooth, elliptical galaxy with a relatively high degree of roundness. It exhibits a bright, concentrated core that gradually fades outwards into a less defined halo. There is no evidence of spiral arms or a distinct disk structure. The color profile suggests a population of older stars, with a yellowish-orange hue dominating the galaxy's light. There are no obvious signs of active star formation, such as blue star clusters or HII regions. The galaxy does not appear to be undergoing any major mergers or tidal disturbances, maintaining a relatively undisturbed, relaxed morphology. The estimated size of the galaxy is approximately 2.5 kpc in radius, suggesting it is a relatively compact system.
