The galaxy appears to be a relatively smooth, elliptical-like system, presenting a centrally concentrated luminosity profile. The overall shape is close to round, lacking a prominent disk structure or significant irregularities. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a redder, possibly older stellar population dominating the core. No significant tidal features or signs of recent major mergers are discernible, suggesting a relatively quiescent evolutionary history. There might be minor disturbances present, but they do not dramatically disrupt the overall smooth morphology. The galaxy exhibits a significant degree of internal homogeneity, with a lack of clear spiral arm structures or distinct star-forming regions readily visible in the image. The light is mostly homogenous. 
