The galaxy presents as a largely featureless spheroid, exhibiting a smooth, elliptical morphology. A bright, concentrated central bulge dominates the overall structure. The luminosity appears highest within the core, gradually decreasing outwards towards the diffuse edges. There is subtle color variation across the galaxy; a slightly bluer hue is observed closer to the center, suggestive of possible ongoing, but subdued, star formation activity. Fainter, reddish features are visible extending away from the central region, possibly indicating an older stellar population or dust absorption. No distinct spiral arm structures or bar features are discernible. The overall roundness of the galaxy is significant; the ellipticity appears low. There is some visual evidence that suggests subtle irregularities or distortions to the overall shape, possibly indicative of a past minor interaction or merger event. The faint extensions are not uniform and might be tidal features.
