The observed galaxy presents a relatively compact structure. Its morphology appears generally smooth, with no readily discernible spiral arms or a prominent bulge. The light distribution seems fairly uniform, with a subtle color gradient from a slightly more bluish center towards a redder periphery. This could indicate a variation in stellar populations or dust distribution. While the overall appearance is smooth, there might be subtle features suggesting minor disturbances or interactions. There is a hint of asymmetry on one side. Further investigation into its velocity field and higher-resolution imaging would be beneficial to determine the nature of any potential merging activity. The galaxy is not particularly bright, suggesting it is either relatively small, distant, or has a lower rate of star formation.
