The galaxy presents as a somewhat smooth, centrally concentrated object. The overall form appears largely spheroidal, with a notable absence of well-defined spiral arms or a distinct disk component. There is evidence of a mild level of disturbance or interaction, potentially suggestive of past or ongoing merging activity. The color profile indicates a relatively evolved stellar population, exhibiting a redder hue, this could indicate the presence of older stars. There may be some level of ongoing star formation. The light distribution indicates it has a luminosity consistent with other massive galaxies at its redshift.
