The galaxy presents a relatively smooth and concentrated morphology. It appears elliptical in shape, with a high degree of central concentration gradually fading into the surrounding space. There is minimal evidence of spiral arm structure or significant dust lanes. The galaxy's color profile suggests a somewhat older stellar population, leaning towards redder hues in the central region, which then fades into blue hues, but very subtly. Indications of any active galactic nucleus are not apparent given the limitations of the image resolution, but given the smooth profile and redder central luminosity, the galaxy is likely an elliptical galaxy, possibly undergoing little or no star formation activity at the present epoch. The lack of any disturbances suggests it has not undergone any major merger events recently. The galaxy is a moderate size, with an estimated radius of 5 kiloparsecs.
