The galaxy presents as a relatively compact object with a noticeable smooth morphology, lacking any distinct spiral arms or bar structures. The light distribution appears centrally concentrated. The color gradient suggests a higher concentration of younger, bluer stars in the central region, surrounded by a more diffuse, redder halo possibly indicating an older stellar population. There is some indication of asymmetry, particularly on the periphery which could indicate minor tidal disturbances or interactions, but it may also be image artifact. The luminosity profile indicates it is likely a massive galaxy with a moderate rate of ongoing star formation.
