The galaxy presents as a relatively compact, moderately bright elliptical object. It exhibits a predominantly smooth morphology with a slight elongation, suggesting a possible deviation from perfect sphericity. The color profile appears bluer towards the central region, gradually transitioning to redder hues in the outer regions. This color gradient might indicate a higher concentration of younger, hotter stars in the galactic nucleus, with older, cooler stellar populations dominating the outskirts. There is a subtle suggestion of possible disturbance in the galaxy's structure but it is likely the presence of an image artifact. No clear signs of spiral arms or a prominent disk are visible.
