This galaxy exhibits an elliptical morphology with a smooth, featureless appearance. It has a predominantly rounded shape. The galaxy appears to be relatively undisturbed, showing no signs of major mergers or significant tidal interactions.

The central region of the galaxy shows a high concentration of light, indicating a prominent nucleus or bulge. The color profile suggests a population of older stars dominating the galaxy's composition, with a yellowish-red hue indicative of a lack of significant ongoing star formation. There is a slight indication of blue light in the disk, suggesting some star formation may be present, although at a low rate. The galaxy is a substantial object, likely with a stellar mass exceeding 10^10 solar masses.
