The galaxy appears as a relatively smooth, elliptical-shaped object. Its color gradient transitions from a bluer periphery to a redder, more concentrated core. This may indicate a difference in stellar populations, with the central region potentially hosting older, redder stars and the outer regions exhibiting some evidence of younger, bluer stars. The general smoothness suggests a well-mixed stellar population and the absence of prominent spiral arms or significant dust lanes. There might be minor disturbances in the outer regions, suggesting possible interactions or minor mergers in its past. The light distribution is not perfectly spherical, appearing slightly elongated in shape. The apparent size is relatively compact for a galaxy, and its overall morphology suggests it is likely an intermediate to massive galaxy in terms of stellar mass.
