The galaxy presents a generally smooth and centralized luminosity profile. It exhibits a moderate ellipticity, appearing somewhat elongated in shape, with the major axis oriented roughly horizontally in this image. The galaxy's color profile indicates a redder central region, possibly suggesting an older stellar population concentrated towards the core. Moving outwards, the color appears to shift slightly toward bluer tones, hinting at the presence of younger stars in the outer regions, although such features are not prominent. There are no readily apparent spiral arm structures or significant dust lane features visible at this resolution, indicating a morphology that appears to be closer to elliptical. There are no major tidal disturbances or signs of ongoing major merger events. The galaxy exhibits a weak signature of star formation.
