The galaxy presents as a largely homogenous, elliptical structure with a smooth luminosity profile, showing a high degree of central concentration. It appears predominantly featureless upon visual inspection, lacking prominent spiral arms, dust lanes, or signs of ongoing major mergers. The galaxy exhibits a generally round morphology, deviating only slightly from a perfect circular shape. There is little evidence of significant tidal disturbances or interactions with neighboring galaxies. Color gradients suggest a redder, older stellar population dominating the galaxy, indicative of limited ongoing star formation. While the central region is bright, there are no signs of an active galactic nucleus in this image, though it is difficult to discern fine detail.
