The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is little evidence of spiral arm structure or significant dust lanes. The galaxy exhibits a primarily yellowish-orange color profile, suggesting a dominant population of older stars and/or significant dust obscuration, though minimal star formation cannot be ruled out. The isophotes appear largely round. There are no apparent signs of a major ongoing merger or significant tidal disturbances. The overall impression is that of an early-type galaxy, potentially an elliptical or lenticular system seen at a relatively high redshift, consistent with its reported size.
