The galaxy presents as a centrally concentrated object with a smooth overall appearance. Its morphology is elliptical, exhibiting a moderate degree of roundness with no discernible spiral arm structures or a prominent disk. The light distribution suggests a gradual decline in stellar density from the core to the outskirts.

A noticeable color gradient exists, shifting from a yellowish core to a bluer periphery. This could indicate either a difference in stellar population with older, redder stars concentrated in the center, or the presence of ongoing star formation in the outer regions. There is no obvious sign of a major recent merger event; instead, only slight disturbances in the light profile are observed. The galaxy's shape does not appear significantly elongated or distorted.
