The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a concentrated central bulge that gradually fades into a less distinct disk. There is a slight elongation. Color gradients are subtle, with a yellowish-white core and a bluer outer region. The galaxy does not appear to be undergoing any major merging events or showing signs of significant tidal disturbances, though there may be some minor irregularities. Star formation appears low, with a population of older stars.
