The galaxy presents as a single, relatively smooth object. The light is concentrated toward the center, suggesting a dense galactic nucleus. The overall color appears to be yellowish-orange, which is a good indication of an older stellar population dominating the galaxy's light output. The galaxy does not exhibit obvious spiral arm structures or dust lanes, lending to a generally elliptical appearance. Given its smooth morphology and color, there seems to be minimal ongoing star formation within the galaxy. There is no evidence of strong tidal features or distortions, which would indicate recent merger activity, although there is a slight irregularity to the shape which could suggest minor interaction.
