The galaxy presents an elliptical morphology, exhibiting a smooth, diffuse light distribution with no readily apparent spiral arms or distinct features. The central bulge is prominent, appearing brighter and more concentrated than the outer regions. The overall color profile suggests a mix of stellar populations, with the central regions displaying a more yellow/red hue potentially indicative of older, cooler stars. Fainter, bluer regions extend outwards, possibly hinting at ongoing, albeit low-level, star formation within the disk. The galaxy appears elongated, exhibiting a cigar-like shape, and displays no obvious signs of interaction or major disturbances, although a subtle asymmetry in the outer regions cannot be ruled out. The lack of clearly defined dust lanes or prominent star-forming regions indicates a relatively quiescent system.
