The galaxy presents a generally smooth, elliptical morphology. The core is highly concentrated and luminous, with a significant decrease in surface brightness observed towards the outer regions. The light distribution appears relatively even, with no strong evidence of spiral arm structures or prominent dust lanes. The galaxy appears to be generally red in color, but shows some variance from core to edge. There is little evidence of recent or ongoing major merger activity, though there may be a hint of minor asymmetry or a slight tidal disturbance.
