The galaxy appears as a relatively compact object with a somewhat irregular morphology. The light profile suggests a bright, concentrated central core region. Extending outward from the core, there is a fainter, more diffuse halo or envelope. Indications of a spiral structure are not immediately apparent. Color gradients are subtle, with the central region exhibiting a bluer hue and the outer regions tending toward a slightly redder color. There is a slight asymmetry in the outer halo, which could potentially indicate tidal disturbance or ongoing minor merging events. However, given the object's smooth appearance overall, any such interaction is likely in a relatively early stage. Further analysis including higher resolution imaging and spectral data is needed to confirm these observations.
