The galaxy presents a generally smooth and elliptical morphology, displaying a concentrated central bulge. The object exhibits a colour gradient, transitioning from a yellowish hue in the core to a slightly bluer tint towards the outer regions, although the colour difference is not significant. There is no visible evidence of spiral arm structures or prominent dust lanes. The overall shape is somewhat elongated but not excessively cigar-shaped. There is no clear indication of ongoing or recent major merger activity, though some minor structural irregularities cannot be ruled out based on this image alone. The faintness of blue light and the mass estimate suggests it is composed of relatively older stellar populations, and has a low star formation rate.