The galaxy appears as a centrally concentrated object, exhibiting a primarily smooth morphology. The light is most intense towards the core, which displays a yellowish hue, possibly indicating an older stellar population. Moving outward from the core, the galaxy displays a gradual decrease in surface brightness and a subtle shift towards slightly bluer colors. This could indicate the presence of more recent star formation in the outer regions, though at a lower rate than in actively star-forming galaxies. There is no obvious spiral structure or bar. The galaxy is moderately elliptical in shape. There is no visual evidence of a major ongoing merger, although there is a subtle asymmetry on one side, possibly indicating a minor interaction or disturbance. Overall, the galaxy presents as a relatively evolved system, with a significant fraction of its stellar mass already formed.
