The galaxy presents a generally smooth morphology, suggesting a system dominated by an older stellar population. The overall shape appears somewhat elliptical, exhibiting a moderate degree of elongation, though tending towards a more rounded form. The central region is noticeably brighter and more concentrated in intensity than the outer regions, indicative of a galactic bulge. There are subtle signs of possible disturbances or asymmetries in the galaxy's structure, potentially indicative of minor tidal interactions or recent accretion events, though its structure is largely undisturbed. The galaxy appears to be a considerable distance, as evidenced by its small angular size and redshift of approximately z = 0.27, suggesting it has intermediate mass with ongoing star formation at a relatively low rate. 
