The galaxy presents a centrally concentrated luminosity profile, exhibiting a smooth, elliptical morphology. The core region displays a yellowish-orange hue, suggesting an older stellar population. The isophotes become slightly more diffuse and redder towards the outer regions. There is no strong evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a galaxy that is well evolved, possibly an elliptical or lenticular type, lacking significant ongoing star formation. Slight color variation is seen towards the periphery. The object appears relatively isolated. There are no obvious signs of tidal disturbances or interactions with nearby galaxies.
