The galaxy presents as an elongated, likely disk-shaped structure, oriented approximately edge-on relative to our line of sight. A prominent central bulge is observed, displaying a concentrated luminosity gradient indicating a high stellar density. The bulge region appears yellowish-white, suggestive of an older stellar population. The surrounding disk exhibits a bluer hue, indicative of ongoing star formation or a younger stellar population, though the color is subtle. There is morphological disturbance in the disk. The general structure indicates a possible recent or ongoing merger event. There is also a smaller galaxy in the bottom right of the large galaxy.