The observed galaxy exhibits a primarily disk-like morphology, albeit with noticeable features deviating from a perfectly smooth structure. The central bulge presents a concentrated luminosity, indicating a significant population of older stars. A spiral arm structure is discernible, though somewhat flocculent and not tightly wound. These arms appear asymmetrical, with one arm exhibiting a more extended reach than the others. Patches of bluer light are distributed throughout the arms, suggesting regions of active star formation. There is evidence of some minor disturbance in the overall morphology, potentially indicative of a past or ongoing minor merger event. The color profile suggests a range of stellar populations, with a tendency towards bluer colors in the outer disk. The galaxy is not currently undergoing a major merger. 
