The galaxy presents a generally smooth morphology. Its overall shape appears elliptical, tending toward round. There is a concentrated central bulge with a high degree of luminosity, transitioning gradually to a less luminous, more diffuse outer region. The color profile appears relatively uniform across the galaxy, with a slightly bluer hue in the central region, suggesting a younger stellar population in the core. No prominent spiral arm structures or dust lanes are discernible. There is a very slight indication of possible tidal disturbance or a minor merger event on its periphery, but the main body shows no signs of major disruption. The galaxy does not appear to be a late-stage merger.
