The galaxy presents as a relatively smooth, elliptical form. The central bulge is prominent and exhibits a bright, concentrated light profile, appearing almost unresolved. The galaxy's color profile suggests a dominant population of older stars, emitting light towards the redder end of the spectrum, though a bluish hue is still slightly discernable. There is a small hint of some possible disturbance in its shape, but this could also be due to the light profile. The lack of well-defined spiral arms or significant dust lanes supports its classification as an early-type galaxy, likely an elliptical or lenticular galaxy viewed close to face-on. Overall, it appears as a mature, relatively quiescent system.
