The galaxy appears to be a relatively smooth, elliptical type. It has a concentrated central bulge that graduates into a less dense halo. There is little indication of spiral arms or significant dust lanes. The galaxy exhibits a generally round shape with a high degree of symmetry. There may be some minor tidal disturbance or interaction influencing its morphology. The colour profile shows a tendency towards redder hues, especially towards the central regions, which might suggest an older stellar population.
