The galaxy presents as an intermediate system, appearing neither entirely smooth nor dominated by prominent features like spiral arms. There is some indication of structure within the galaxy, possibly faint, diffuse features. The shape is largely in between a perfectly round morphology and an elongated, cigar-like shape. The galaxy appears to be experiencing some disturbances in its overall morphology, potentially indicating minor gravitational interactions or internal dynamics. There is no strong evidence of a major merger. The luminosity suggests the galaxy is a fairly luminous object, actively forming new stars.
