The galaxy appears to be a relatively smooth, single structure with a concentrated central bulge. The light distribution suggests an elliptical morphology, with the isophotes appearing close to circular. There are no obvious spiral arms or bar features visible. 

A color gradient is present, with the central region exhibiting a yellow-orange hue. This suggests an older stellar population dominates the core. Moving outwards from the center, the color transitions to a bluer tone, indicative of younger, hotter stars contributing to the outer regions. The galaxy shows hints of possible minor disturbances in its shape, but overall presents as a fairly relaxed system.
