The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears centrally concentrated with a bright, yellowish core region, suggesting a significant population of older stars. The outer regions of the galaxy are less defined and exhibit a gradual fading in intensity, with subtle color variations indicating a mix of stellar populations. There is no obvious disk structure or spiral arms, and no clear evidence of strong tidal disturbances or ongoing major mergers are apparent. There may be some signs of minor disturbances. The overall morphology suggests a galaxy undergoing relatively low levels of star formation. The object has intermediate roundness, appearing neither perfectly circular nor excessively elongated.
