This galaxy appears to be a relatively small, elliptical galaxy, exhibiting a smooth, concentrated morphology. Its color profile indicates a spectral shift towards the red end of the spectrum, suggestive of an older stellar population. The galaxy’s light is centrally concentrated, with a rapid decrease in intensity moving outward from the core, showing little to no spiral arm structure, and a generally featureless structure. There is no obvious evidence of active star formation. It is a galaxy with a generally round profile. No signs of merging or other galaxy interactions are visible in this image.
