The galaxy presents a morphology consistent with a spiral galaxy, exhibiting distinct spiral arm structures. The arms appear flocculent, and tightly wound around a prominent central bulge. The color profile shows bluer hues within the spiral arms, suggestive of ongoing star formation activity. A moderate bar structure may exist, though it is not clearly defined. The bulge displays a yellowish hue indicating the presence of an older stellar population. No signs of a major merger are present, but there is an asymmetric pattern of light distribution that may be a possible minor interaction or disturbance occurring on one side of the galaxy.
