The galaxy presents as a relatively compact object, exhibiting a somewhat irregular morphology. There is evidence of a central, brighter region, potentially a galactic nucleus. Surrounding this core, the distribution of light suggests a more extended structure, albeit without a clearly defined disk or spiral arm morphology. Some asymmetry can be observed, possibly indicative of gravitational interactions or recent merger activity.

Color gradients are subtle but present, with a tendency for bluer hues in the outer regions, which may suggest younger stellar populations. The central area appears slightly redder, potentially indicative of older stellar populations or dust obscuration. The integrated light suggests that the system exhibits a mid-range luminosity. The overall appearance seems to suggest that this is a moderately sized galaxy that could be in the process of merging or has experienced a recent interaction, which might explain its irregular shape and subtle color variations.
