The galaxy presents as a somewhat elliptical or lenticular structure, appearing relatively smooth in texture. The central region exhibits a higher concentration of light, suggesting the presence of a galactic bulge. The light appears yellowish-white, indicative of an older stellar population. Moving outward from the core, the surrounding disk region displays a more diffuse, bluish-white hue, possibly pointing to ongoing star formation within the galaxy. There is a slight asymmetry observed in the overall structure, hinting at the possibility of either a minor gravitational interaction or perhaps some internal dynamic process affecting the distribution of stellar populations. No strong dust lanes or distinct spiral arms are discernible from the image. Overall, the galaxy appears to be in a relatively quiescent state, with evidence of both old and potentially young stellar populations contributing to its observed luminosity.
