The galaxy presents as a relatively smooth and rounded structure, exhibiting a concentrated central region which appears brighter than the surrounding area. This region transitions into a more diffuse halo. The overall color profile suggests a mixture of stellar populations. The central area appears slightly redder in hue, possibly indicating older stars, while the outer regions show a hint of bluer tones, suggesting the presence of younger stars or ongoing star formation at a low rate. There are no distinct spiral arms or a prominent disk structure visible. There are no signs of major disturbances, tidal tails, or obvious ongoing merger activity. Overall, the galaxy appears to be a relatively quiescent system.
