This galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light distribution without prominent spiral arms or distinct features. Its shape is elongated, appearing cigar-shaped, with a high degree of ellipticity. The central region is brighter and more concentrated, suggesting a dense stellar population or active galactic nucleus. The color gradient transitions from a reddish-orange core to slightly bluer outer regions, potentially indicating differences in stellar populations with older stars concentrated centrally and younger stars more dispersed in the outskirts. There is no obvious evidence of ongoing major mergers or significant tidal disturbances in the galaxy's morphology. The overall impression is of a relatively undisturbed, evolved system.
