This galaxy exhibits a predominantly smooth morphology with a suggestion of a disk-like structure. The central region displays a concentrated, bright core, indicative of a substantial stellar population or potentially an active galactic nucleus. Moving outward from the core, the galaxy's luminosity gradually decreases, transitioning into a fainter, more diffuse halo. The overall color profile suggests a relatively evolved stellar population, with a redder hue concentrated in the central regions, possibly indicating older stars or a higher dust content. A subtle bluer component is present in the outer regions, possibly indicating younger stellar populations. There is no obvious sign of tidal tails or major disturbances, although there is a hint of some asymmetries, possibly suggesting a past minor merger event or some internal dynamism. The galaxy appears moderately elliptical in shape. The star formation appears moderate, with the majority occuring in the outer areas.
