The galaxy appears as a moderately bright, centrally concentrated object. It exhibits a yellowish hue, suggesting an older stellar population. The galaxy's morphology is largely smooth, with no prominent spiral arms or bar structures visible. It is mostly elliptical in shape, tending towards a slight ellipticity rather than being perfectly circular. There is no evidence of major mergers or significant tidal disturbances; the galaxy appears relatively undisturbed. Faint, diffuse extensions may be present, but the resolution limits definitive assessment. Overall, the galaxy presents as a relatively quiescent, mature system.
