The galaxy presents as a slightly tilted disk galaxy. A prominent, moderately sized bulge dominates the central region, exhibiting a yellowish hue suggestive of an older stellar population. Fainter spiral arm structures extend from the central bulge, displaying a bluer color, which is indicative of ongoing star formation. There is no clear bar structure. The overall morphology suggests that the galaxy is neither a recent merger nor currently undergoing significant interaction, although some minor disturbances cannot be ruled out. The disk appears to be in the process of forming stars, while the central bulge is more settled and likely composed of older stars. There are no signs of an edge on disk. 
