The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a dominant central bulge that appears quite round and concentrated, with a gradual fading in luminosity towards the outer regions. The color profile suggests an older stellar population, indicated by the yellowish-red hue. There is no apparent spiral arm structure or significant dust lane obscuration visible in this image. The overall morphology leans towards a quiescent system, potentially indicative of low star formation activity. Some subtle irregularities on the edges may imply minor gravitational interaction, but there is no major merging activity detected.