The galaxy appears to be a relatively smooth, elliptical system with a concentrated central bulge. There's a subtle color gradient, with the core exhibiting a slightly yellower hue, suggesting an older stellar population. Fainter, bluer regions extend outwards, possibly indicating some ongoing, albeit subdued, star formation in the galaxy's outskirts. The galaxy shows a generally round morphology. There is no obvious indication of a major merger, although there appears to be a slight disturbance within the galaxy disk.
