The galaxy appears as a moderately bright, elliptical-shaped object. It is centrally concentrated with a smooth luminosity profile, suggesting an evolved stellar population. The galaxy exhibits a yellowish-orange hue, indicative of older stars and a lack of significant ongoing star formation. There are subtle irregularities in the outer regions, possibly indicating minor tidal disturbances or interactions with smaller satellite galaxies. There's a hint of bluer light on one side of the galaxy, which may be due to recent star formation. Overall, the galaxy presents a morphology characteristic of a massive elliptical galaxy, but shows some evidence for past or ongoing mergers.
