The galaxy presents as a relatively compact object with a somewhat irregular morphology. It appears largely amorphous, lacking a distinct spiral arm structure or a clearly defined central bulge. Color gradients are subtle, with a general trend towards bluer tones. There is no bright central concentration of light. The galaxy does not exhibit any obvious signs of major mergers, though minor disturbances may be present. It is moderately luminous, with a smooth appearance that does not strongly suggest ongoing, intense star formation.
