The galaxy presents a mostly smooth, elliptical morphology. Its light is concentrated towards the center, exhibiting a bright, well-defined core. The overall color appears somewhat redder, suggesting an older stellar population and relatively low levels of ongoing star formation. The galaxy appears to be slightly elongated in shape. There is no obvious presence of spiral arms, dust lanes, or significant tidal disturbances. The galaxy does not appear to be undergoing any major merging events. There may be a slight minor asymmetry but is imperceptible.
