The galaxy presents as a single, relatively smooth concentration of light. Its morphology appears elliptical, showing a central bulge that decreases in surface brightness gradually towards the edges. No distinct spiral arms or features indicative of active star formation are readily apparent. The galaxy exhibits a color profile that is slightly redder at the core and bluer towards the outer regions. The overall shape is roughly circular. There is no evidence of any ongoing major merging events or strong tidal disturbances affecting the structure of the galaxy, although there is some minor asymmetry visible. 
