This galaxy appears to be a relatively face-on spiral with a prominent bulge. The bulge is characterized by a bright, concentrated region of light, suggesting a high density of older stars. The disk surrounding the bulge exhibits a relatively smooth, diffuse structure. There is a faint suggestion of spiral arms, though they are not well-defined. Some features may indicate minor disturbances. The overall color suggests a galaxy with a mix of stellar populations, with a relatively modest rate of star formation. 
