The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge with a yellowish hue, indicative of an older stellar population. The light profile decreases gradually from the core, transitioning into a less defined, extended halo region with a subtle blue tinge. There is no evident spiral arm structure or bar. The galaxy's overall appearance suggests minimal ongoing star formation. No signs of major disturbances due to mergers or tidal interactions are apparent. The shape appears to be more in between round and elliptical, but closer to round.
