The galaxy presents as a relatively compact, smooth object with a roughly circular morphology. There is a dominant central bulge that appears mostly featureless, with a somewhat indistinct edge. The galaxy displays a noticeable color gradient, appearing bluer in the central regions, potentially indicating a population of younger, hotter stars. The outer regions are marginally redder. There are no strong indications of prominent spiral arms, bars, or significant dust lanes visible in this image. The overall light distribution suggests a primarily elliptical or lenticular classification. There is some minor disturbance that could suggest a small interaction with a nearby galaxy, but this is minimal.
