The galaxy presents as an elliptical morphology, with a significantly brighter central bulge. The luminosity appears to decrease gradually from the core outwards, lacking distinct spiral arm features. The color gradient across the galaxy suggests an older stellar population, with the central bulge exhibiting a yellow-orange hue, indicative of evolved stars. There's little evidence of blue star formation regions. The galaxy appears relatively undisturbed, with no signs of tidal tails or major morphological distortions indicative of a recent merger event. The overall shape is somewhat elongated, but not excessively so.
