The galaxy appears to be a relatively smooth, elliptical system. It presents with a concentrated central bulge and a diffuse halo. The light distribution is highly centrally concentrated, with the majority of the luminosity emanating from the core. Color gradients are subtle, but there's a hint of a redder hue towards the galaxy's center, potentially indicating an older stellar population. There is a notable absence of distinct spiral arms or significant dust lanes. The galaxy's overall shape is roughly circular, displaying a high degree of symmetry. No significant tidal features or signs of major ongoing mergers are immediately apparent, though there appears to be minor disturbances in the galactic disc. Given the apparent roundness and lack of prominent disk-like features, this system likely falls into the early-type galaxy classification.
