The galaxy presents a somewhat elliptical morphology, appearing mostly smooth with a concentrated central bulge exhibiting a yellow-white hue, indicative of an older stellar population. Fainter, bluer, diffuse extensions are visible surrounding the central region, possibly suggesting ongoing, but relatively subdued, star formation within the galactic disc. These extensions appear asymmetrical, indicating possible interactions, although no major distortions or tidal features are readily apparent. Overall the galaxy's appearance suggests a system transitioning from a spiral to elliptical morphology, potentially via secular evolution or minor mergers. The galaxy is not a perfect elliptical, but displays a high degree of central concentration and lack of distinct spiral arms.
