The galaxy presents a somewhat irregular morphology, appearing neither purely elliptical nor a well-defined spiral. There is evidence of both a smooth, centrally concentrated component and fainter, more diffuse features extending outward. The color profile suggests a mix of stellar populations. A central bluish hue is visible, which could be associated with younger, hotter stars indicating some level of ongoing star formation. The outer regions show a slightly redder tint, suggestive of older stellar populations. Overall, the galaxy appears relatively compact, with a fairly low surface brightness. It seems to be an evolving system, possibly undergoing interactions or internal processes that are disrupting any pre-existing disk-like structure. The smooth, centrally concentrated area could be a bulge, and is surrounded by regions of patchy, less organized star formation.
