The galaxy presents an overall elliptical morphology, although it's elongated shape suggests a possible disk component viewed at an oblique angle. The central region exhibits a bright, concentrated nucleus, indicating a high stellar density in the core. Moving outwards from the core, the galaxy displays a gradual decrease in luminosity. The color profile reveals a yellowish hue in the central bulge region, consistent with an older stellar population. Fainter, bluer regions are observed in the outer disk, hinting at ongoing star formation. There is no clear evidence of strong spiral arm structure or prominent dust lanes. The overall smooth appearance suggests it might be in a late stage of its evolution, possibly transitioning towards a lenticular or elliptical galaxy type, though there is minor evidence of a possible past merger event. 
