The observed galaxy presents as a moderately compact object. It displays a generally diffuse morphology, with a subtle elongation that suggests a possible disk-like structure, although it is not sharply defined. The central region appears slightly brighter than the outer regions, possibly indicating a concentration of older stellar populations, though this is not definitive. There is evidence of some irregularities in the galaxy's structure, possibly indicating tidal interactions with another galaxy, or perhaps recent merger activity. These appear as faint extensions of the main body of the galaxy. The overall color profile of the galaxy suggests a mix of stellar populations. The central region is subtly redder, while the outer regions may exhibit slightly bluer hues, potentially reflecting a difference in the age and composition of the stars in these regions. There is a low probability of the galaxy being a relatively undisturbed spiral or elliptical galaxy, but a higher probability of it being a later stage merger or a disturbed disk galaxy.
