The galaxy appears to be a relatively small, elliptical system. Its morphology is primarily smooth, lacking any prominent spiral arms or distinct disk features that would classify it as a spiral galaxy. The light distribution is fairly concentrated and uniform, suggestive of an older stellar population, although there is some visible color variation across the galaxy's body. The galaxy's shape is highly circular and has no apparent signs of significant tidal disturbances or ongoing major merging events. Some minor asymmetry or disturbance is not ruled out. There may be a faint, diffuse halo extending slightly beyond the main body of the galaxy.
