The galaxy presents as a spiral type, observed at an oblique angle relative to our line of sight. A prominent central bulge dominates the structure, exhibiting a smooth, concentrated luminosity profile. It appears yellow-white in color. Fainter spiral arms extend outwards from the bulge, displaying a bluer hue, suggestive of ongoing star formation. These arms appear relatively tightly wound around the central bulge. The galaxy does not show strong evidence of a recent major merger, but may be undergoing minor disturbances that influence its morphology. The galaxy displays a bar-like structure that seems to be quite significant within the inner region. The disk of the galaxy shows signs of dust lanes within the spiral arms. The spiral arms appear flocculent in nature, with high levels of star formation throughout.