This galaxy exhibits a moderately elliptical morphology, appearing somewhat elongated but not excessively so. The central region displays a bright, concentrated bulge, suggesting a significant population of older stars. Progressing outwards from the core, a smoother, more diffuse disk is observed, albeit with a low level of discernible structure. Faint spiral arm structures are tentatively detected upon close inspection, but their definition is not prominent, possibly due to the viewing angle or the galaxy's morphological classification. The colour gradient transitions from a yellow-orange hue in the central bulge to a subtly bluer tint in the outer disk regions. This colour shift hints at potential ongoing star formation in the outer regions, relative to the bulge's older stellar population. Overall, the galaxy appears to be a relatively massive system, with a moderate rate of star formation activity. There is no obvious indication of major mergers or significant tidal disturbances. The disk is not perfectly flat, showing subtle warps or thickening along its major axis.
