The galaxy presents as a centrally concentrated, elliptical or lenticular type. It is relatively smooth in appearance, lacking prominent spiral arms or distinct dust lanes. The light distribution is centrally concentrated, with a bright, yellowish core suggesting an older stellar population. The outer regions of the galaxy gradually fade into the background, with a subtle halo extending beyond the bright central region. There is minimal evidence of ongoing star formation, as indicated by the lack of blue or ultraviolet light. There is no sign of any major or minor mergers, though there are some minor disturbances that have been observed, it appears to be a relaxed system.
