The galaxy presents a morphology consistent with a spiral type. Two prominent spiral arms are discernible, exhibiting a moderately wound structure. The bulge appears to be of moderate size, with a high concentration of luminosity towards the center. The galaxy does not seem to be undergoing a major merger, though the possibility of a minor disturbance is not completely ruled out. The overall color suggests a mix of stellar populations, with the central bulge displaying a yellower hue, potentially indicating older stars. There is no evidence for an edge-on disk or strong bar structure, but there is evidence of a weaker bar. The spiral arms exhibit regions of bluer light, suggestive of recent star formation. The disk is visible and not very disturbed.
