The galaxy exhibits a generally smooth morphology, appearing as a central bulge with a slightly elongated disk. The overall color profile suggests a population dominated by older stars, giving it a yellowish-orange hue. There is a subtle blueish tinge at the edges of the disk, possibly indicating a small population of younger, hotter stars. No distinct spiral arm structures or dust lanes are readily apparent. It presents as an elliptical or lenticular galaxy, with a relatively high degree of central concentration. It shows no obvious signs of ongoing major mergers or strong tidal disturbances.
