The galaxy appears as an elongated, elliptical structure with a smooth, diffuse light distribution. The central region exhibits a brighter, yellowish hue, suggesting an older stellar population. Fainter, bluer tones are visible toward the outer regions of the galaxy, potentially indicating more recent star formation in these areas. Overall, the galaxy seems to be relatively undisturbed, showing no obvious signs of major mergers or strong tidal interactions. The shape appears to be elongated, but not extremely so, indicating a moderate degree of ellipticity.
