The galaxy presents as a centrally concentrated object with a bright, diffuse core. There is a distinct, somewhat amorphous halo extending outwards from the central region. The overall morphology appears relatively smooth, lacking well-defined spiral arms or a prominent bar structure. The color profile suggests a higher concentration of blue light in the central regions, possibly indicating ongoing star formation. Fainter, redshifted light appears in the outer regions of the halo. There is a slight asymmetry in the overall shape, with a subtle extension or distortion noticeable on one side, potentially indicative of a past or ongoing interaction with another galaxy, though no distinct companion is readily visible in this image. Further spectroscopic analysis would be beneficial in determining the nature of the light distribution and overall galactic composition.
