The galaxy appears as a centrally concentrated, luminous object. The light profile seems relatively smooth, with a high degree of central concentration. The overall shape approximates a rounded spheroid. There is a slight color gradient, with a yellowish hue in the central region, transitioning to a slightly bluer color in the outer parts. There is no clear indication of spiral arm structure or a distinct disk, although the slight variation in color could indicate low-level disk features. No apparent major disturbances or merging features are discernible, although slight asymmetries in the outer regions may indicate minor tidal interactions or internal disturbances. The estimated physical size, combined with the inferred mass and star formation rates, suggest that this galaxy is a relatively massive system with moderate on-going star formation activity. The smooth morphology further suggests that this is likely a moderately evolved system.
