The galaxy presents as a somewhat compact object with a relatively smooth, centrally concentrated light distribution. The core exhibits a bright, possibly unresolved region. There is a subtle extension of light beyond the core, which appears almost spheroidal. Some asymmetric structure exists in the form of faint irregularities or extensions, possibly indicating minor disturbances. The overall morphology does not suggest a grand design spiral or a well-defined elliptical shape, but leans more towards a featureless or disturbed system. Based on the color distribution, the core appears to be bluer than the outer regions, which seem to be redder, suggestive of a difference in stellar populations and/or dust content. 
