The object appears to be a galaxy exhibiting a moderately smooth morphology. The light distribution suggests a primarily elliptical or lenticular form, with a high degree of central concentration. The galaxy displays a yellowish hue in its central region, transitioning to a bluer tint at its periphery. There is evidence of a possible ongoing merger or tidal interaction, given the disturbed morphology and asymmetrical light distribution. One can see a second distinct luminous area that is connected to the primary body of the galaxy. The galaxy's shape is generally round, though it has some minor irregularities. The presence of these features would seem to indicate ongoing or recent interactions with another galaxy.
