The galaxy presents as a somewhat elongated structure. Its overall morphology appears disturbed, possibly indicative of a merger event or tidal interaction. There is a suggestion of two distinct nuclei or areas of concentrated luminosity within the galaxy's core, further supporting the possibility of an ongoing or recent merger. The color profile suggests a relatively old stellar population with possibly suppressed star formation, with a bias toward redder wavelengths. Patches of bluer light suggest regions of younger, hotter stars.
