This galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and centrally concentrated light distribution. The morphology suggests a relatively evolved system, characterized by a dominant spheroidal component. The galaxy presents a diffuse halo, gradually fading into the background sky. There is a subtle elongation to the galaxy's overall shape, being slightly more "in-between" in roundness, rather than purely spherical. There are no obvious signs of spiral arms or significant dust lanes, which further supports its classification as an elliptical galaxy. There may be some evidence of minor interaction or disturbance, but no major mergers are evident. The galaxy has a small angular size. The apparent color appears to be in the blue to white range, corresponding with old star formation.
