The galaxy presents as a relatively small, well-defined structure. Its overall morphology appears smooth, lacking prominent spiral arms or distinct features suggestive of active star formation regions. The light distribution is centrally concentrated, indicating a prominent bulge. The shape appears somewhat elongated, resembling a cigar shape rather than being perfectly round. There is no obvious indication of a major ongoing merger or significant tidal disturbances. The light is slightly reddish suggesting an older stellar population and relatively low star formation rate.
