The galaxy presents an elliptical morphology with a noticeable central bulge. The light distribution appears smooth and concentrated towards the core, with a gradual decrease in intensity towards the outer regions. A faint, extended disk-like structure is suggested, oriented horizontally in the image. There is a subtle variation in color across the galaxy, with the central region exhibiting a more yellowish hue, possibly indicating an older stellar population, while the outer regions appear slightly bluer. The galaxy exhibits a generally undisturbed form, with no obvious signs of a major merger. There may be minor disturbances or faint tidal features in the periphery but they are difficult to distinguish with clarity. Overall, the galaxy seems to be relatively evolved, potentially representing a transitional phase between a spiral and an elliptical type.
