The galaxy appears as a centrally concentrated elliptical structure, exhibiting a smooth, luminous profile. The core region presents a bright, yellowish-white hue, indicating a population of older stars. The light diffuses outwards, transitioning to a fainter, greenish tint in the outer regions. There is no apparent disk structure or spiral arms visible, and the galaxy appears generally undisturbed with no strong evidence of recent merger activity or significant tidal distortions. There are very faint, diffuse areas outside the main structure of the galaxy, which are likely faint galaxy stars in the halo. Overall, the galaxy shows characteristics consistent with a mature elliptical galaxy.
