The galaxy presents an elliptical morphology, appearing largely smooth and featureless. Its color profile suggests a relatively old stellar population, with a dominant yellowish-orange hue concentrated towards the central bulge. There is little evidence of spiral arm structure or active star formation regions. The overall appearance is consistent with an early-type galaxy, possibly an elliptical or lenticular galaxy viewed at a considerable distance. A slight asymmetry is observed in the outer regions, potentially hinting at minor tidal interactions or past merger events. However, no strong disturbances or merging features are readily apparent. The galaxy displays a central concentration of light intensity, decreasing outwards in a gradual manner.
