The galaxy appears as a moderately bright, elliptical-shaped object. It exhibits a relatively smooth and diffuse light distribution, lacking prominent spiral arms or distinct features typically associated with disk galaxies. There may be a faint central bulge or core region displaying a slightly brighter and more concentrated emission compared to the outer regions. The overall color of the galaxy appears to be on the redder side, possibly indicating an older stellar population with a lower rate of ongoing star formation. However, there are hints of bluer light suggesting that there may be some star formation present. The galaxy shows little evidence of major tidal disturbances or mergers, but slight asymmetries may imply minor gravitational interactions or internal dynamic processes. Its roundness also suggests it may have a smooth shape, which may indicate that it has a relatively homogenous distribution of stars within its structure.
