The galaxy presents a largely smooth, elliptical morphology. The central bulge is prominent and appears relatively spherical, exhibiting a concentrated luminosity profile. There may be some minor disturbances within the galaxy but overall it appears generally undisturbed, without obvious spiral arm structures or a well-defined disk. The galaxy presents a yellowish hue, suggestive of an older stellar population and lower star formation rate. The object appears to be relatively massive, with a calculated diameter of roughly 7 kpc.
