The galaxy presents as a moderately luminous object at a redshift of approximately 0.369. It exhibits a generally smooth morphology, with a significant fraction of the light concentrated in a spheroid. There is evidence of minor disturbances, possibly indicative of past interactions or ongoing minor merger events. The galaxy has a relatively high estimated stellar mass. The central region displays a bright, somewhat diffuse light profile, potentially suggesting an older stellar population. The overall color is consistent with a galaxy in which star formation is suppressed, although the luminosity is indicative of ongoing processes. The galaxy's shape is close to round.
