The galaxy presents as a centrally concentrated object with a bright, roughly spherical core. There is evidence of a surrounding, less luminous structure which appears somewhat irregular and elongated. The galaxy displays a color gradient, with the core exhibiting a bluer hue compared to the outer regions, which tend toward a redder appearance. There may be a minor interaction or disturbance, as suggested by the slight asymmetry in the outer structure. Though the image quality is limited, the overall morphology does not appear to be that of a classic spiral or elliptical galaxy, but may be disturbed.