The galaxy presents a centrally concentrated morphology. The core region exhibits a bright, unresolved nucleus, suggestive of significant ongoing activity or a supermassive black hole.  The radial intensity profile decreases from the core outwards, but not perfectly smoothly. There appears to be some clumping of light in an area to the left of the core, though the light is faint.

The overall color of the galaxy appears slightly blue-green, suggestive of ongoing star formation, but the high central concentration also suggests an older population is dominant. The light distribution is not perfectly symmetrical, appearing slightly elongated and lumpy to the side of the core region, which may indicate minor interaction with another galaxy. There is no visual evidence of strong spiral arms or a well-defined disk structure.
