The galaxy appears to be a relatively smooth and elliptical galaxy. The core exhibits a concentrated yellowish hue, suggesting a population of older stars. A subtle color gradient extends outward from the core, transitioning into a bluer disk-like structure. This indicates the presence of some younger stars or ongoing star formation, albeit at a lower rate. The galaxy's shape is elongated, exhibiting a notable cigar-shaped morphology rather than a perfectly circular structure. There is no obvious evidence of major mergers or significant tidal disturbances in the galaxy's immediate vicinity. The overall structure suggests a dynamically evolved system.