The galaxy presents as a generally smooth, centrally concentrated object. It exhibits a nearly circular morphology with a high degree of symmetry. No prominent spiral arms, bars, or significant dust lanes are discernible. The light distribution suggests a relatively uniform stellar population across the galaxy, with a gradual decrease in luminosity moving outwards from the core. There is a hint of color variation, with the central region exhibiting a slightly yellower or redder hue compared to the outer regions, which appear somewhat bluer. This could indicate an older stellar population in the core and relatively younger populations in the outskirts. There is no obvious evidence of ongoing or recent major mergers or tidal interactions, although subtle disturbances cannot be entirely ruled out. Overall, the galaxy appears to be a relatively massive, quiescent system with a low star formation rate.
