The galaxy presents as a smooth, centrally concentrated object with a noticeable bulge. Its overall shape appears to be elliptical, exhibiting a moderately round morphology. There is little evidence of distinct spiral arms or significant disk-like features. The galaxy's color profile suggests a dominance of older stellar populations, giving it a yellowish hue. Faint extensions or disturbances may be present, hinting at possible past interactions or minor mergers, but the galaxy appears largely undisturbed in its current state. There is very little evidence of on-going star formation.
