The galaxy presents a smooth, elliptical morphology. The central region displays a concentrated, bright core with a yellowish hue, suggesting a population of older stars. Moving outward from the core, the light gradually diminishes, transitioning into a slightly bluer halo. The shape is moderately elongated, appearing closer to round than cigar-shaped. There is no clear evidence of spiral arms or significant dust lanes. The general smooth and symmetric appearance suggests minimal signs of recent major merger activity or strong tidal disturbances, though subtle, minor interactions cannot be ruled out. The overall color profile indicates ongoing, though perhaps subdued, star formation activity within the galaxy.
