The galaxy presents as an elliptical-like structure, though there is some suggestion of a flattened disk. The light distribution appears relatively smooth, with a concentrated central bulge exhibiting a yellowish hue, indicating an older stellar population. The outer regions display a bluer tinge, which could signify the presence of younger, hotter stars, although dust obscuration cannot be ruled out as a contributor to the color. The galaxy’s shape deviates from a perfect circle, exhibiting a slight elongation. There is no obvious evidence of strong spiral arm structure or prominent dust lanes. The overall morphology suggests a system in a relatively quiescent state, possibly transitioning from a spiral to a more elliptical form, or having undergone a past merger event that has largely settled. Further spectroscopic analysis would be needed to verify the galaxy's star formation rate and confirm the age of the stellar populations in different regions.
