The galaxy presents as a somewhat elongated, smooth structure with a bright central region. The light profile appears to decrease gradually from the center outwards. There is a slight asymmetry, appearing more extended along one axis, suggestive of a possible elliptical morphology. Faint and diffuse outer regions suggest a gradual decline in stellar density as distance from the galactic center increases. The color appears generally consistent across the galaxy, trending toward the redder end of the spectrum. There is no clear evidence of spiral arms or significant dust lanes based on this image. Based on the morphology classification, this galaxy is likely an elliptical galaxy. Slight disturbances may be present but are minor.
