The observed galaxy presents a centrally concentrated luminosity profile with a smooth, spheroidal morphology. The core appears bright and slightly off-white, indicating a concentration of older stellar populations. Emanating from the central region, there's an extension that looks like a 'tail'. This exhibits a more diffuse, orange-red hue. The overall shape suggests the possibility of a galaxy undergoing a minor merger event or tidal disruption, evident in the observed luminosity extension. While the central region shows a relatively smooth appearance, the presence of the observed feature indicates ongoing or recent gravitational interaction. Further analysis through multi-band photometry and spectroscopy is necessary to confirm the nature and composition of the observed extension.
