The galaxy presents as a somewhat diffuse, disk-like structure, approximately 9 kiloparsecs in diameter based on estimated parameters. A bright central bulge is visible, exhibiting a yellowish hue, suggestive of an older stellar population. Faint, ill-defined spiral arm structures appear to emanate from the central region. The arms exhibit a mottled texture with a faint bluish color that suggests ongoing star formation. The overall morphology is suggestive of an intermediate-type spiral galaxy. Based on the observed characteristics, the galaxy appears to be a mature system undergoing moderate star formation, with a possibility of minor disturbance based on the overall structure. Further spectroscopic analysis would be beneficial to determine precise star formation rates and confirm merger activity.
