The galaxy appears to be an elliptical or lenticular type, displaying a largely featureless, smooth morphology. The object exhibits a radial concentration of light, with intensity peaking at the galactic center. The color appears generally red, indicative of an older stellar population and a lower rate of ongoing star formation. There is no discernible spiral arm structure or dust lane attenuation. Slight asymmetry may suggest minor gravitational interaction or recent accretion events. The round appearance indicates minimal disk dominance.
