The galaxy presents a generally smooth morphology. It appears elliptical in shape, though is approaching a more circular form. The central region exhibits a high concentration of light, indicative of a dense stellar population or active galactic nucleus. The color is predominantly yellow, suggesting a population of older stars, but also appears to be undergoing star formation, as implied by the blue/green hue of the outskirts, albeit at a low rate. There is minimal evidence of distinct spiral arms or a well-defined disk structure. The overall structure is largely undisturbed, with no obvious signs of recent major merger events, though there are minor disturbances suggesting possible ongoing interactions with smaller galaxies. The galaxy extends for a considerable distance in its observed location.
