The galaxy presents an overall elliptical morphology, appearing predominantly smooth and lacking prominent spiral arm structures. The central bulge is bright and concentrated, exhibiting a yellowish hue which likely indicates an older stellar population. The galaxy gradually fades toward its periphery, lacking a distinct edge. There is a slight elongation observed, though the galaxy is primarily rounded in appearance, without significant distortions suggesting a major ongoing merger. The absence of strong blue colors suggests a relatively low star formation rate. There is a very slight disturbance to the lower right of the galaxy, possibly indicating a minor interaction. 
