The galaxy presents a largely smooth morphology. It is moderately elliptical in shape. The light distribution suggests a central bulge that is moderately bright and concentrated. There is evidence of some internal structure within the galaxy, but it lacks well-defined spiral arms or a prominent disk. There is a color gradient; the central region appears whiter, gradually shifting to bluer hues in the surrounding regions. This may imply on-going or recent star formation in the outer regions. The overall color indices indicate that the galaxy consists of middle-aged and older stellar populations with only a modest star-forming regions. The galaxy shows no clear signs of major mergers or tidal distortions. There may be evidence of a minor disturbance.
