The galaxy exhibits a generally smooth morphology, appearing largely spheroidal in shape. There is a concentrated central bulge that dominates the overall light profile, radiating outwards into a less-defined halo region. The color appears to be relatively uniform, with a yellowish hue that suggests an older stellar population, with little evidence of significant recent star formation. There are no obvious signs of spiral arms, bars, or other disk-like features. Overall, the galaxy is reasonably well-defined, without major disturbances or evidence of active merging.
