The galaxy exhibits a primarily elliptical morphology, with a smooth appearance overall, though not entirely uniform. The central region shows a higher concentration of luminosity, suggestive of a bulge. While the overall structure is smooth, there is some subtle suggestion of a faint, diffuse disk component.

A faint arm-like feature might be present at one end, showing a possible sign of disturbance, but it could also be an artifact. Overall, the galaxy appears relatively isolated and shows no strong indication of major merger activity, though some minor disturbances cannot be ruled out. The color profile is consistent with an older stellar population, indicating a mature galaxy. The galaxy is moderately bright with a slightly reddish hue.
