The galaxy presents a generally smooth and somewhat elliptical morphology. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. Moving outward, the galaxy displays a diffuse halo with a gradual decrease in surface brightness. Overall, the galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. The distribution of light suggests a more evolved stellar population. The color distribution indicates a redder central region transitioning to a more bluish halo. This color gradient could be indicative of ongoing star formation in the outer regions of the galaxy. A secondary, smaller region of light is visible on the upper right of the galaxy. It is unknown if this is part of the galaxy, or another object entirely. It does however appear to be a similar color to the center of the main galaxy body.
