The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy with minimal discernible spiral arm structure. The central region exhibits a higher concentration of light, indicating a bulge component that dominates the overall luminosity. The galaxy appears elongated, deviating somewhat from a perfectly circular profile. The color of the galaxy is predominantly yellow-orange, indicating an older stellar population with lower rates of ongoing star formation. There is a slight suggestion of a tidal disturbance or a minor interaction with a companion galaxy.
