The galaxy presents as a relatively compact and centrally concentrated object. Its overall morphology appears largely smooth, suggesting a dominant spheroidal component. However, there is an apparent slight extension or distortion to one side of the galaxy's core, which could indicate a minor tidal interaction or internal disturbance. The color profile shows a subtle bluer tint particularly in that extended region. This suggests the presence of some on-going star formation. The galaxy's light distribution appears generally uniform across the main body. There is no clear evidence of spiral arms, a prominent disk, or a strong central bar within the limits of this image's resolution.
