The galaxy presents as a spiral type, exhibiting a well-defined disk structure. Evident spiral arms emanate from a central bulge region. The bulge appears relatively prominent and concentrated, displaying a yellowish hue suggestive of an older stellar population. The spiral arms themselves showcase a bluer color, indicating the presence of younger, hotter stars and ongoing star formation. The arms appear somewhat flocculent in nature. Hints of dust lanes are visible within the spiral arms, obscuring some of the background starlight. The galaxy is seen at a slight inclination, offering a partial view of the galactic disk. There may be a weak bar structure near the center. No evidence of strong tidal disturbances or major merger events is immediately apparent.
