The galaxy presents a somewhat amorphous morphology, appearing more featureless than structured. A central, highly luminous region dominates the galaxy's appearance. This core exhibits a bright, almost stellar-like concentration of light. Surrounding this central core is a fainter, more diffuse halo of light, extending outwards in a roughly elliptical shape. The light distribution within the halo appears uneven, with subtle variations in brightness. There is a slight extension to one side that may indicate a tidal arm or possibly a smaller galaxy being tidally disrupted. The overall color gradient suggests a higher concentration of younger, bluer stars in the central region, with a gradual shift towards redder hues in the outer halo, potentially indicating an older stellar population there. There is some suggestion of minor disturbances visible within the galactic structure.
