The galaxy presents as a generally smooth, elliptical structure with a discernible central bulge. Its shape is somewhat elongated, appearing somewhere between round and cigar-shaped, with its longest axis oriented roughly horizontally in the frame. The color distribution is fairly uniform across the galaxy, with a slightly bluer hue towards the center, suggesting the potential for some ongoing, albeit subdued, star formation in the core region. There is no evidence of spiral arms or a well-defined disk. No major disturbances or signs of an ongoing merger event are readily apparent in the galaxy's morphology, although the structure is not perfectly smooth and may have experienced a minor interaction in the past. The outer regions appear to fade gradually into the background sky, indicating a relatively diffuse halo. Overall, the galaxy appears to be a moderately sized, relatively quiescent system.
