The galaxy presents as a relatively smooth, elliptical or lenticular structure. The central bulge is bright and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. The surrounding disk, extending outwards from the bulge, displays a bluer color, indicative of ongoing or recent star formation. There is a slight asymmetry or disturbance visible in the outer regions of the disk, possibly resulting from a minor gravitational interaction. The overall shape is somewhat elongated but generally smooth, with no prominent spiral arms or bar structures immediately apparent. The galaxy's integrated light suggests it is moderately luminous.
