The galaxy appears as a centrally concentrated object with a smooth morphology. The light distribution suggests a predominantly spheroidal shape, exhibiting a noticeable elongation along a preferred axis. The color profile indicates a bias towards blue wavelengths. A central, brighter region is present, surrounded by a fainter, diffuse halo of similar color. There is no clear evidence of spiral arms or a distinct disk structure within the available resolution. There does not appear to be any active merging or tidal disturbances.
