The galaxy appears to be a relatively smooth, elliptical or lenticular type, exhibiting a centrally concentrated bulge region. The light profile fades gradually from the core outwards, indicating a lack of prominent spiral arms or distinct features associated with active star formation in a disk. The overall shape is largely circular. There is some hint of redder hue toward the outer edges. No clear evidence of tidal tails, major distortions, or recent merger activity is apparent. There is a possible indication of a very minor disturbance or irregularity in the galaxy's morphology. 
