The galaxy presents as a slightly elongated, elliptical shape, with a smooth, diffuse light distribution. There is a subtle color gradient from the center outwards, exhibiting a yellowish-white core that transitions to a bluish hue in the outer regions. No distinct spiral arm structures or dust lanes are discernible in this image. There are no signs of prominent tidal features or ongoing major mergers, indicating a relatively undisturbed morphology. The overall appearance suggests a galaxy dominated by an older stellar population, particularly within the central bulge, with some recent or ongoing star formation occurring in the outer regions, contributing to the bluer colors observed there. The galaxy's elongated shape points towards a possible S0-type classification.