The galaxy presents a generally smooth, elliptical morphology, with no prominent spiral arms or bar structure visible. The light distribution is concentrated towards the center, forming a bright, yellowish core, which fades into a less defined halo. The galaxy appears somewhat elongated, showing a slight deviation from a perfectly circular shape. There is no evidence of ongoing major mergers or significant tidal disturbances, though there could be a minor interaction. The object's overall color suggests an older stellar population.
