The galaxy presents as a relatively smooth, elongated structure, suggestive of an elliptical morphology, although a highly inclined disk galaxy cannot be ruled out. The central region exhibits a brighter, more concentrated luminosity profile compared to the outer regions. There is little to no evidence of prominent spiral arms or significant dust lanes. The color appears largely uniform, with a subtle bluish tint, potentially indicating the presence of some younger stellar populations. However, the dominance of redder wavelengths is still apparent. There is a subtle hint of minor disturbances or asymmetries in the morphology, possibly indicative of past or ongoing interactions. However, the disturbances do not appear to be strong. 
