The galaxy appears as a slightly elongated spheroid with a concentrated central region. The light distribution is relatively smooth, lacking distinct spiral arms or prominent features. The color gradient shifts from a bluer core to a redder periphery, indicating a possible transition in stellar populations, with younger stars concentrated in the central region and older stars populating the outer parts. The shape is close to circular, yet slightly flattened. There is no clear evidence of active galactic nuclei, merging activity, or significant dust lanes from this image alone. Overall, the galaxy presents a morphology consistent with an early-type galaxy, potentially an elliptical or lenticular galaxy, as opposed to a spiral.