The galaxy appears as a moderately sized, centrally concentrated object. It presents a generally elliptical morphology, although with some deviation from a perfect ellipse.

The light distribution suggests a relatively smooth profile, lacking strong, well-defined spiral arms or a prominent bar structure. There is a subtle color gradient across the galaxy, transitioning from a slightly bluer hue in the central regions to a redder hue in the outer halo. This could indicate variations in stellar populations, with younger, bluer stars dominating the core and older, redder stars populating the outskirts. Faint disturbances are visible in the halo. 
