The galaxy presents as a relatively smooth, elliptical-like structure, elongated along one axis, with an apparent high degree of central concentration. There's a distinct color gradient observable, with a yellowish-white core transitioning to a redder periphery. No obvious spiral arm structures or prominent dust lanes are discernible within the limits of image resolution. The object exhibits a fairly symmetrical morphology, with only the slightest hint of possible disturbance or tidal features present. It appears as an isolated system within its immediate field. The overall luminosity suggests it is a massive galaxy, likely containing a significant population of older stars. The redder color towards the outer regions may indicate an older stellar population with lower star formation activity.
