The galaxy presents a generally elliptical morphology, exhibiting a smooth, featureless appearance with a high degree of central concentration. The core is a bright, diffuse yellowish-white, indicative of an older stellar population. Moving outward from the core, there is a subtle decrease in luminosity, fading to a faint blueish-white glow. The overall shape is somewhat elongated but primarily round, with no apparent spiral arm structures or significant dust lanes visible in this observation. There may be minor signs of disturbance present, though the dominant impression is of a relaxed system. The color gradients suggest a centrally concentrated distribution of older stars and potentially lower rates of recent star formation throughout the galaxy.
