The galaxy appears to be a relatively compact object, exhibiting a generally smooth morphology. There is little evidence of significant spiral arm structures or a pronounced disk component. The galaxy presents a near-spherical shape. No obvious signs of ongoing or recent major merger events are observed, although subtle disturbances cannot be ruled out. The color profile suggests a population of older stars, with a possible contribution from ionized gas, giving it a blue/green hue in the center of the object. The overall appearance is consistent with that of an elliptical galaxy, or perhaps a lenticular galaxy seen face-on.
