The galaxy appears as an elliptical-like object. The light is concentrated towards the center, with a smooth, gradual decline in brightness moving outwards. The central region exhibits a yellowish hue, indicating the presence of older stellar populations. There is little evidence of spiral arms or significant dust lanes. The galaxy's overall shape is elongated, resembling a cigar shape rather than a perfect sphere, but is classified as being in between this shape and round. There are no obvious signs of a major ongoing merger or significant tidal disturbances in the immediate vicinity of the galaxy, although some evidence of minor disturbances may be present. The object's morphology suggests an evolved system with a relatively low star formation rate.
