The galaxy presents a largely smooth morphology, with a slightly elliptical shape. There is a strong concentration of light towards the center, suggesting a significant bulge component. The color profile indicates a redder core, possibly indicative of an older stellar population or dust obscuration. Fainter, diffuse light extends outwards from the core, with no apparent spiral arm structure or distinct features. The overall appearance is consistent with an early-type galaxy, likely an elliptical or lenticular galaxy at an approximate distance corresponding to a redshift of z=0.31. There are hints of a possible minor disturbance in the outer regions, though no clear merging activity is apparent.
