The galaxy appears to be an elliptical or lenticular type, exhibiting a generally smooth light distribution. Its morphology is largely featureless, suggesting a well-mixed stellar population. There may be some slight evidence of a disk, but the galaxy is dominated by a spheroidal component. The galaxy exhibits a slight elongation along a roughly horizontal axis. Its color profile indicates a population of older stars, with the core exhibiting a yellowish-white hue. Some blue light exists, hinting at a small degree of on-going star formation. There is no evidence of any major merging events occurring within the galaxy.
