The galaxy exhibits a flattened, elliptical morphology, appearing as a cigar-shaped spheroid. The color distribution suggests a concentration of older stellar populations towards the central region, indicated by the reddish hue. Progressing outwards from the core, a subtle color gradient towards a bluer tone is discernible, potentially indicative of ongoing or recent star formation within the galaxy's disk. There are no clearly defined spiral arms or bar structures visible. The general smoothness of the light distribution suggests the absence of significant ongoing merging activity or major tidal disturbances. A minor asymmetry or faint disturbance might exist.
