The galaxy presents as a relatively smooth, centrally concentrated object, appearing largely spheroidal in shape. The light distribution suggests a high degree of rotational symmetry. There is little evidence of spiral arm structures or significant dust lanes. Its color appears consistent with an older stellar population, exhibiting a reddish hue. Some faint asymmetry is detected, possibly indicative of a minor gravitational interaction or past merger event. The galaxy appears to be a rather luminous object at its redshift, given its relatively compact size. There is no apparent active galactic nucleus visible in the image, nor any significant HII regions suggesting active ongoing star formation.
