The galaxy presents as a relatively smooth, elliptical-like structure. Its core is a bright, concentrated yellow-white, suggesting an older stellar population. The overall shape is nearly round, with no apparent strong asymmetries or tidal features. The color gradient transitions from a bright, yellowish core to a more diffuse, reddish-yellow halo, indicating a possible decrease in stellar age and/or metallicity with increasing radius from the center. There are no distinct spiral arm structures visible, and the overall morphology suggests a system dominated by random stellar motions rather than organized rotation. There is very slight blue around the edges. The galaxy exhibits low star formation rates, based on the redder color and lack of prominent blue star-forming regions.
