The galaxy appears to be a relatively compact, elliptical system exhibiting a smooth, mostly featureless morphology. The light distribution suggests a centrally concentrated spheroid with a high degree of symmetry. There is little evidence of spiral arms or a prominent disk structure. The galaxy possesses a yellowish-red hue, potentially indicative of an older stellar population and a low rate of on-going star formation. There are no obvious signs of active galactic nuclei (AGN) activity, major mergers, or significant tidal disturbances. A subtle asymmetry is apparent on one side, potentially indicating a very minor interaction or internal structure.
