The galaxy presents an overall elliptical morphology, exhibiting a smooth, relatively featureless appearance. Its color profile suggests a dominant population of older stars, indicated by the yellowish-orange hue concentrated towards the galactic center. There is a subtle color gradient from the central region outwards, with the outer edges appearing slightly redder, which could be indicative of either an older stellar population in the outskirts or dust obscuration. There is a faint disk-like structure, but it's difficult to determine the inclination with certainty. There is no apparent strong spiral arm structure, and no signs of active star formation regions are visible. No significant tidal tails or distortions are immediately apparent, suggesting the absence of a recent major merger event. Given the overall smooth appearance, it is likely an evolved galaxy in relative isolation.
