The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that appears bright and has a bluish-white color, suggesting active star formation. The outer regions of the galaxy display a gradual decrease in luminosity, transitioning from bluish-white to a yellowish-red hue, possibly indicating an older stellar population with less on-going star formation. There are no obvious spiral arm structures or significant dust lanes visible. The galaxy appears undisturbed, with no signs of recent major mergers or tidal distortions. The overall morphology suggests an early-type galaxy with a dominant spheroid component.
