This galaxy presents as a fairly luminous, centrally concentrated object. It appears largely smooth in texture, lacking any prominent spiral arm structures or a distinct galactic bar. The light distribution is characterized by a high degree of radial symmetry, with the isophotes appearing generally elliptical. There may be some minor disturbances or asymmetries within the outer regions of the galaxy's halo, but nothing that strongly indicates a major ongoing merger event. There appears to be a notable lack of intense, localized star-forming regions. The galaxy exhibits a moderate redshift, suggesting a significant distance from our own galaxy.
