The galaxy presents as a moderately inclined disk system, appearing somewhat elliptical in shape with a noticeable bulge. The central bulge exhibits a yellowish hue, indicative of an older stellar population. The disk component displays a bluer color profile, suggesting the presence of ongoing star formation. There is a subtle asymmetry to the disk, with a slight elongation on one side and a possible minor disturbance in morphology, but does not appear to be a major merger event. The galaxy's outer regions seem diffuse and ill-defined.
