The galaxy presents as a centrally concentrated object with a somewhat smooth morphology. There appears to be a slight elongation in its overall shape. The central region displays a bright, yellowish-white core, suggesting an older stellar population. The outer regions exhibit a bluer hue, potentially indicative of more recent star formation activity. There may be some minor disturbances in the galaxy's structure, particularly in the outer regions where the light distribution is less uniform. Overall, it appears to be a galaxy undergoing some level of ongoing star formation.
