The galaxy appears to be a relatively compact object with a dominant central bulge. The light is concentrated towards the center, suggesting a high stellar density in that region. The color profile indicates the presence of older stellar populations, likely with diminished recent star formation. There are hints of a very faint, diffuse disk surrounding the bulge, but any spiral arm structure is subtle or absent. The overall shape is somewhat elliptical, but approaching a spherical morphology, as opposed to a flattened disk-like structure. There is a very subtle asymmetry visible in the outer regions, potentially indicating a minor interaction or disturbance. The galaxy doesn't show any strong evidence of a major ongoing merger, though there's some subtle evidence of it having happened sometime in the past.
