The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated core, suggesting a high density of stars in this area. Moving outward from the core, the light gradually diffuses, forming a halo of diminishing brightness. The overall color profile appears to be dominated by older stellar populations, presenting a yellowish-red hue. There's no clear evidence of spiral arms, dust lanes, or significant star formation regions in the visible spectrum. The galaxy appears largely undisturbed, with no obvious signs of recent mergers or tidal interactions.
