The galaxy presents a somewhat elliptical morphology, appearing relatively smooth in structure with a lack of distinct spiral arms or a central bar. The core exhibits a concentrated, bright luminosity, suggestive of a significant stellar population or possibly an active galactic nucleus, though further spectroscopic data would be needed to confirm the latter. The light from the galaxy appears to be somewhat redder than that of surrounding field stars. The galaxy shows a slight elongation, deviating moderately from a perfect circular form. No obvious tidal features or signs of recent major mergers are visible in this image.
