The galaxy presents a generally smooth morphology, with a notable elongation along its major axis. The light distribution suggests a spheroidal component dominates the overall structure, indicating it may be an elliptical galaxy, or a lenticular galaxy seen edge-on. There may be a small disk component, but its presence is difficult to discern. The color gradient transitions from a bluer hue at one end to a redder, more yellow hue towards the center, which is more prominent than the end. Overall the galaxy appears to be reasonably massive. Based on the asymmetric structure, the galaxy may be undergoing some minor gravitational disturbance through a minor merger or tidal interaction.
