The galaxy presents a predominantly smooth and rounded morphology. The central region exhibits a high concentration of light, appearing bright and yellowish-white, suggesting an older stellar population. There is a noticeable radial decline in luminosity from the center outward, transitioning to a fainter, more reddish hue in the outer regions. No distinct spiral arm structures or prominent dust lanes are visible. The galaxy appears relatively undisturbed, showing no clear signs of major mergers or tidal disruptions. A minor asymmetry is present in the outer envelope, possibly indicating a previous minor interaction. Based on the color profile and smooth structure, the galaxy is likely an elliptical galaxy with a considerable mass and low rate of star formation.
