The galaxy exhibits a generally elliptical morphology, appearing largely smooth and rounded. The central bulge is prominent and displays a yellowish hue, suggesting an older stellar population with reduced ongoing star formation. Moving outward from the core, the galaxy appears bluer, indicative of more active star formation in the disk. There is a subtle hint of spiral arm structure, but they are not well-defined, suggesting either a flocculent spiral pattern or a galaxy transitioning towards a more lenticular shape. The galaxy's light profile is relatively concentrated, with luminosity decreasing gradually from the core outwards. There is no evidence of significant tidal disturbances or ongoing mergers based on its symmetric and undisturbed appearance. Overall, the galaxy appears to be a transition type, possibly between a spiral and an elliptical.
