The galaxy presents a moderately bright, centrally concentrated luminosity profile, indicative of a significant central bulge component. The overall morphology appears to be transitioning from smooth to a weak spiral structure. There is an indication of a faint disk, but the arms are not well-defined. Some irregularities are observed in its shape, which might be attributed to minor gravitational interactions or internal dynamics. These interactions suggest that the galaxy may be undergoing or may have recently experienced a merger event. The galaxy appears to be a relatively luminous object at its redshift, suggesting it is a massive system, with evidence of recent star formation.
