This galaxy presents a disk-like morphology with a central bulge. The disk is oriented at a moderate inclination relative to our line of sight, allowing for a partial view of its structure. Prominent spiral arms extend from the central bulge, displaying a loosely wound structure. The arms show a mottled appearance suggesting regions of active star formation along their length. The galaxy exhibits a color gradient, with bluer tones in the spiral arms indicating the presence of younger, hotter stars, while the central bulge appears yellower. There are indications of a possible bar structure. The overall structure appears to be somewhat disturbed. The galaxy does not appear to be undergoing a major merger.
