The galaxy appears as a centrally concentrated object with a smooth, diffuse morphology. The light distribution is largely symmetrical and lacks prominent spiral arms or bar structures. There's a subtle color gradient visible, with a slightly bluer hue towards the central region, potentially indicating a modest amount of on-going star formation, although it's not extensive. The overall appearance is dominated by light from older stellar populations. The galaxy presents a relatively round shape, suggesting it is not viewed edge-on. There is no obvious evidence of major tidal disturbances or ongoing mergers. Faint, subtle irregularities in the outer regions may suggest a history of minor interactions, but the galaxy appears largely relaxed and undisturbed.
