The galaxy appears as a single, centrally concentrated object with a smooth, elliptical morphology. Its core is very bright, with light appearing in the yellow region. It shows a notable decrease in surface brightness as it extends away from the central region, fading into a blueish color. There is no evidence of spiral arms or a prominent disk. Subtle irregularities might be present, but the overall structure suggests a well-mixed stellar population and a lack of significant ongoing mergers or tidal disturbances. The round shape may imply that it is an elliptical galaxy, and its smooth structure may indicate an older stellar population. The gradient may imply star formation is higher at the core, or that there is a supermassive black hole with an accretion disc. There is no evidence of any major disturbances or merging activity.
