The galaxy appears as a centrally concentrated, elliptical-like structure. The core region exhibits a bright, smooth luminosity profile, characterized by a yellowish-white hue, suggesting an older stellar population. The outer regions appear less luminous, with a gradual decrease in intensity outwards. There appears to be a slight elongation, making it unlikely to be perfectly round. There are no obvious spiral arm structures or prominent dust lanes visible in this image. The overall morphology suggests a relatively undisturbed system. No signs of significant ongoing or recent merger activity are apparent.
