The galaxy presents a morphology dominated by a smooth, centrally concentrated structure. The light profile indicates a relatively high degree of symmetry, tending towards a round shape. The galaxy displays a central bulge that emits strongly, with a gradual decrease in luminosity extending outwards. There are hints of a faint disk structure. Overall, the galaxy appears undisturbed, without any obvious signs of recent major mergers or significant tidal interactions. The general color profile leans towards a redder hue, suggesting an older stellar population, and a relatively low rate of star formation.
