This galaxy presents as a centrally concentrated, relatively smooth object. The light distribution suggests a dominant spheroid component. The shape appears largely elliptical, with a slight elongation, and could be described as being between round and cigar-shaped. There are no obvious signs of major disturbances or ongoing mergers visible in this image, with most citizen scientists classifying the galaxy as "not merging".

The color profile shows a general yellow hue with an indistinct inner region. This suggests the stellar population is mostly composed of older stars, with lower star formation rates. The galaxy appears quite massive.
