The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape appears to be somewhat elliptical, though tending towards round. The light distribution is dominated by a bright central region, with a gradual decrease in intensity moving outwards from the core towards the diffuse edges. There is no obvious spiral structure, bar, or other distinct features. The color is generally consistent across the galaxy, with subtle variations in hue, perhaps indicating variations in stellar populations, however, there are no obviously discernible star-forming regions. The overall morphology does not indicate any major interactions or mergers, though a slight asymmetry cannot be ruled out, implying past minor gravitational disturbance.
