The galaxy presents an elliptical morphology, appearing largely smooth and spheroidal in shape. There is a notable concentration of light towards the galactic center, suggestive of a significant bulge component. The overall color of the galaxy appears relatively blueish, possibly indicating the presence of younger stellar populations. However, the outer regions show a slight shift towards redder hues, which may imply a higher proportion of older stars within those areas. There are no prominent spiral arms or dust lanes visible in this image. There appears to be some minor disturbances in the galaxy's overall structure, suggesting a potential interaction with another galaxy or recent merger event.