The galaxy presents as a luminous, elliptical morphology. The core exhibits a concentrated brightness, diminishing gradually toward the outer regions. There is a noticeable lack of distinct spiral arm structure or prominent dust lanes. The overall color profile leans toward the redder end of the spectrum, with a prominent yellow-orange hue in the central bulge, suggesting an older stellar population. Fainter, bluish regions are subtly observed in the extended halo, hinting at some ongoing, albeit subdued, star formation. The galaxy appears relatively undisturbed, with no signs of major mergers or significant tidal distortions.
