The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology with a high degree of roundness. There is a distinct color gradient, with a bright, yellowish-white core that gradually transitions to a dimmer, reddish halo. No obvious spiral arm structures or dust lanes are discernible in this image. The overall appearance suggests a lack of significant ongoing star formation activity. There is no evidence of major mergers or tidal disturbances in the immediate vicinity. The galaxy appears to be a relatively isolated system, undisturbed by interactions with nearby galaxies.
