The galaxy presents a primarily smooth, elliptical morphology. It exhibits a high degree of central concentration, with luminosity gradually decreasing outwards from a bright, unresolved core. The overall color profile appears relatively uniform, trending toward the redder end of the spectrum. There is a slight elongation of the galaxy along a specific axis, indicating a deviation from perfect circularity. No distinct features such as spiral arms, dust lanes, or tidal tails are discernible. The galaxy appears undisturbed, with no evidence of recent or ongoing merger activity. The image suggests a relatively old stellar population dominating the galaxy's light output.
