The galaxy appears to be a relatively smooth, centrally concentrated object. It exhibits an elliptical or lenticular morphology, lacking defined spiral arms or a prominent disk structure. The light distribution suggests a dominant spheroidal component. The color gradient indicates a relatively red population of stars, possibly indicating an older stellar population with reduced ongoing star formation. The overall structure is fairly regular, with no obvious signs of major mergers or tidal disturbances, although there could be minor distortions in its overall shape. The galaxy displays a general roundness, with a subtle deviation from a perfect circle. There may be some low level active galactic nuclei activity based on its color and form.
