The galaxy presents as a well-defined elliptical structure, exhibiting a smooth morphology with minimal discernible features such as spiral arms or prominent dust lanes. Its shape appears elongated, with the major axis significantly exceeding the minor axis. The light distribution is centrally concentrated, displaying a radial gradient from a bright, reddish core outward to fainter, bluer peripheries. The core region exhibits a redder color index relative to the outer halo. There is no readily apparent evidence of ongoing major merger activity, although there may be some minor disturbances that are not obvious in this view. The galaxy has a significant mass and a moderate rate of star formation.
