The galaxy presents as an object with a predominantly smooth morphology. The light profile appears concentrated toward the center, suggesting a spheroidal or elliptical structure rather than a distinct spiral disk. It exhibits a moderate ellipticity, appearing neither perfectly circular nor highly elongated. There is evidence of a slight asymmetry or disturbance in the outer regions, possibly hinting at a minor interaction or merger event in its past. While the main body of the galaxy is smooth, there is a faint extension or tidal feature emanating from one side, suggesting a potential gravitational interaction. The galaxy's color suggests a population of older stars, with no prominent signs of active star formation. The overall structure appears to be relatively undisturbed, although subtle features indicate a complex evolutionary history.
