The galaxy appears to be a relatively compact system, likely a disk galaxy seen at an oblique angle, based on the elliptical shape of the central region. There is evidence of a central bulge component, as indicated by the higher concentration of light. The colors indicate the presence of older stars, seen as a redder hue, centrally located. The fainter halo of greenish light surrounding the central bulge is likely younger stars and gas. The edges of the disk are slightly disturbed in appearance, with one side appearing slightly more extended or warped than the other, though the disturbances are likely minor. There is a possible faint arm-like structure or tidal tail emanating from one end, further indicating a possible past interaction. The galaxy appears to be isolated with no sign of any companions that may be the source of these disturbances. 
