The galaxy presents as a relatively smooth, elliptical object, appearing more elongated than perfectly circular. Its light profile suggests a higher concentration of older stellar populations. A slight reddish-yellow hue dominates the central region, indicating a diminished rate of star formation and enrichment of older, redder stars. There's a suggestion of a very faint and diffuse outer halo, but this could easily be lost in the background noise. No distinct spiral arms or prominent dust lanes are immediately visible. There's no evidence of any major ongoing mergers or significant tidal disturbances. Based on the overall morphology, it is likely an elliptical galaxy somewhere between E4 and E6.
