The galaxy presents an elliptical morphology, exhibiting a smooth, centrally concentrated light distribution. The primary body of the galaxy appears elongated, approximately three times longer than it is wide. The central region displays a yellowish hue, suggestive of an older stellar population, while the outer edges show a faint bluish-green tint, potentially indicating the presence of younger, hotter stars and possible star formation activity. There are no visible spiral arms or bar structures, and no obvious signs of a recent major merger, though the slight asymmetry could indicate minor gravitational interactions or disturbances. Overall, the galaxy appears to be a relatively massive system with ongoing, albeit subdued, star formation in the outer regions.
