The galaxy presents as a disk galaxy, observed nearly edge-on. There is evidence of a central bulge, appearing somewhat bright and round. The disk exhibits a smooth, elongated structure. The overall color profile suggests a higher concentration of older stellar populations, with redder hues dominating the galaxy's light output. There are no obvious signs of ongoing major mergers or tidal disturbances, however there may be minor disturbances. The disk appears relatively uniform in color and texture.
