The observed galaxy presents a morphology consistent with a spiral galaxy, although the disk is not sharply defined. There is evidence of spiral arm structures, though they appear somewhat flocculent rather than grand design. A central bulge is discernible, contributing significantly to the overall luminosity of the galaxy; it appears to be of moderate size. The galaxy exhibits a color gradient, with the bulge region appearing more yellow/white in color, suggesting an older stellar population. The disk shows bluer hues, indicative of ongoing star formation. There is no obvious distortion suggestive of a major merger event, but some minor disturbances or asymmetries may be present, meriting further investigation. The galaxy's overall structure suggests an intermediate stage in its evolution. The galaxy has a considerable apparent size. 
