This galaxy appears as a diffuse, somewhat amorphous object. The light distribution is centrally concentrated, fading outwards gradually, with no clear spiral arm structures or bar features visible. The overall shape is moderately elliptical rather than perfectly spherical, with a hint of elongation along one axis.

The color profile suggests a mixed stellar population. There is a generally yellowish or redder hue implying the presence of older stars across the body of the galaxy, with hints of bluer components scattered within the central region of the galaxy, possibly indicating regions of ongoing or recent star formation. There is a slight asymmetry in the light distribution, with one side appearing slightly more extended or disturbed than the other, this may indicate a minor gravitational interaction or merger event.
