The galaxy presents a generally smooth, rounded morphology. A bright, concentrated central bulge is apparent, appearing almost spheroidal. The surrounding disk appears relatively featureless, with a lack of distinct spiral arm structure. There is a subtle color gradient observable, transitioning from a yellower hue in the central bulge to a bluer tone in the outer regions of the disk. No significant tidal disturbances or merger remnants are clearly visible, although there might be very minor asymmetries within the disk suggestive of a weak interaction. The overall impression is of a galaxy that is primarily dominated by an older stellar population.
