The galaxy presents as a spiral galaxy with a moderate bulge. The disk exhibits spiral arm structures that are somewhat flocculent. The central bulge displays a yellowish hue, potentially indicative of an older stellar population. The spiral arms show a bluer coloration, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy does not appear to be strongly barred. There is no morphological indication of a major merger event, although minor disturbances cannot be ruled out from this image alone. The galaxy's shape appears somewhat elliptical. The inner disk exhibits a brighter, more condensed profile, gradually fading toward the outer edges.
