The galaxy presents a predominantly smooth and rounded morphology. The central region exhibits a high degree of luminosity, indicating a concentrated stellar population or possibly an active galactic nucleus. The light appears to be brightest in the blue/white portion of the spectrum, indicating recent or ongoing star formation. There is some visible color variation, with a shift towards redder hues in the outer regions, likely representing an older stellar population. There are no readily apparent signs of spiral arm structure or other distinct features typically associated with disk galaxies, though there are hints of asymmetric distributions in the color suggesting some disruption. No signs of major mergers or tidal tails are immediately visible. The overall appearance is consistent with an elliptical galaxy at an approximate redshift of 0.119.
