The galaxy presents a generally smooth, elliptical morphology. A central bulge is prominent, exhibiting a concentrated luminosity profile with a reddish-orange hue. The galaxy is surrounded by a fainter halo. There may be very faint structures indicating a possible disk. There does not appear to be any ongoing merging events or strong tidal disturbances. The roundness of the galaxy suggests it is not a highly inclined disk galaxy. The overall color indicates that this galaxy is likely composed of older stellar populations.
