The object appears to be a galaxy, exhibiting a largely smooth and elliptical morphology. The light profile suggests a centrally concentrated bulge component with a gradual decrease in luminosity towards the outer regions. The core of the galaxy exhibits a distinct reddish hue, possibly indicative of an older stellar population. Surrounding the core is a region of somewhat bluer light, indicating the possibility of some ongoing star formation. The galaxy displays no obvious spiral arm structures or prominent dust lanes within the resolution limits of the image. The overall shape is close to circular, with a slight elongation, indicating an elliptical type galaxy. There might be a very slight distortion on one side, suggesting a possible minor interaction.
