The galaxy presents a generally elliptical morphology, appearing somewhat elongated along its major axis. The central region exhibits a brighter, more concentrated luminosity, suggesting the presence of a significant galactic nucleus. The overall color profile indicates a bluer hue, particularly towards the outer regions, possibly indicative of ongoing star formation. Although the galaxy appears mostly smooth, there are hints of faint, diffuse structures within the disk, though these are not sharply defined. No significant signs of major disturbances or mergers are apparent, although subtle asymmetries might suggest minor interactions. The galaxy is predominantly an elliptical shape with the possibility of a disk shape within. It is mostly blue in hue, possibly suggesting active star formation.
