The galaxy presents as an elliptical morphology, exhibiting a smooth, somewhat spherical structure. The core region is notably luminous, suggesting a concentration of older stellar populations. Its color profile trends toward the redder end of the spectrum, indicative of a lack of significant ongoing star formation within the main body.  There is also evidence of a faint tidal tail or streamer extending from the galaxy, potentially suggestive of past interactions or accretion events. Despite the general smoothness, some subtle color variations are discernible, hinting at possible substructure within the overall elliptical envelope.
