The galaxy presents as a somewhat diffuse, elliptical-like structure with an overall smooth appearance. The central region exhibits a concentrated luminosity. The galaxy shows a distinct bimodal color distribution, with one region appearing yellowish and another region appearing reddish. This color difference suggests variations in stellar populations or dust content across the galaxy. There's a distinct possibility of an ongoing or recent merger event, given the non-uniform structure. The galaxy doesn't exhibit strong spiral arm features. It may be undergoing significant star formation, though that is difficult to determine based on the image alone. There is a hint of tidal distortion in the galaxy's morphology, supporting the possibility of gravitational interaction.
