The galaxy presents as a single, concentrated object. Its morphology appears largely smooth, with a somewhat elliptical, but largely circular profile. The radial color gradient suggests a central concentration of older stellar populations, exhibiting a yellowish hue, while the outer regions display a slightly bluer tint, suggestive of younger stars. There may be evidence of weak tidal features or minor disturbances, but the overall impression is that of a relatively settled system. Star formation activity appears to be relatively low throughout the galaxy.