The galaxy presents a generally elliptical morphology, appearing more disk-like than spheroidal. The central bulge region exhibits a high surface brightness, transitioning outwards to fainter regions. There is likely a disk component, with an approximately 37% chance that it is edge-on. There are indications of spiral arms, particularly a faint, diffuse feature on one side, indicating a disk structure. There may be some disturbances in the morphology, but no major interactions or mergers are occurring. Overall, the galaxy appears to be a disk galaxy with a bright nucleus. Colors appear bluer towards the outer regions and redder towards the central region, suggesting active star formation in the outer disk and older stellar populations in the bulge.