The galaxy presents as a slightly elongated, disk-shaped structure. The central region exhibits a brighter, yellowish hue, possibly indicative of an older stellar population. Moving outwards from the center, the disk becomes bluer in color, suggesting the presence of younger stars and ongoing star formation, especially in the disk. The galaxy appears relatively undisturbed, with no major signs of mergers or tidal distortions visible. It seems to have a smooth overall structure, with subtle indications of some disk-like components. The galaxy's light distribution seems to be centrally concentrated, without any prominent spiral arms or bar features immediately apparent.
