The galaxy appears to be a relatively compact and centrally concentrated system, with a generally elliptical morphology. The overall color is somewhat redder than a typical spiral, suggesting an older stellar population. The light distribution is generally smooth, lacking any strong evidence of spiral arms or a distinct disk structure. The galaxy's isophotes appear roughly circular. There may be a very slight hint of some disturbance in the galaxy's shape. No obvious merger activity or tidal tails are visible.
