The galaxy appears to be a relatively smooth, elliptical galaxy with a bright, concentrated core. The central region exhibits a yellowish-white hue, indicative of an older stellar population. The galaxy's overall shape is roughly round with a slight elongation. There are hints of faint, diffuse features or arms extending outwards from the core, but they are not well-defined. The color gradients suggest minimal ongoing star formation within the central regions. The galaxy does not appear to be undergoing any major merging events or significant disturbances.
