The galaxy presents as a diffuse, elliptical-like structure with a smooth, largely featureless morphology. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic nucleus or bulge. The overall color appears to be reddish, which could indicate an older stellar population and potentially lower ongoing star formation rates. There is evidence of possible minor disturbances or interactions in its morphology with an elongation or slight irregularity in its shape. There is a strong central concentration of older stars. There is a hint of a potential tidal tail or disturbed structure.
