The galaxy presents as a relatively compact object, exhibiting a predominantly smooth morphology. Its shape approximates a circular form, though a slight elongation is discernible along one axis. Color gradients suggest a concentration of older stellar populations towards the central regions, indicated by a reddish hue. Moving outward, bluer tones become more prevalent, suggesting regions of active star formation. There is faint evidence of a possible disturbance in the galaxy's structure, though whether this is a minor interaction or inherent to the galaxy's formation is not immediately clear. No distinct spiral arms or bar features are readily apparent. Overall, the galaxy appears to be well-defined, without any clear signs of recent major mergers.
