The observed galaxy presents as a relatively compact object with an apparent elliptical morphology. A bright, concentrated central bulge dominates the galaxy's structure. Surrounding the bulge, a fainter, more diffuse halo is visible, exhibiting a subtle gradient in intensity extending outwards. There appear to be some faint features, and the disk has a slight inclination. The overall color profile suggests a moderate population of older stars, with a hint of bluer light indicative of younger stellar populations within the disk. I do not suspect any major ongoing merging events, but there is a slight possibility that there is some minor disturbance in the symmetry.
