The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology, with approximately 82% of the citizen scientists reporting that it is smooth. It is not perfectly circular. It has a slight ellipticity, leaning slightly toward an intermediate shape, and does not resemble a cigar shape. There is little evidence of any major or minor disturbances and therefore no indication that it is actively merging with another galaxy. The light is primarily shifted towards the redder bands, suggesting an older stellar population and relatively low ongoing star formation. The central region appears more concentrated with a brighter, more defined core, possibly indicating the presence of a central bulge.
