The object appears to be a galaxy exhibiting a morphology somewhere between elliptical and disk-like, with a dominant smooth component. The galaxy presents a somewhat elongated profile, deviating from perfect sphericity. While a prominent central bulge or nucleus is not distinctly visible, the light distribution suggests a concentrated core region. There may be some subtle disturbances to the overall structure, indicating a potential interaction or past merger event. This disturbance appears to be a minor interaction. No strong spiral arms or distinct disk features are readily observable. The galaxy's color appears to be consistent across its visible extent.
