The galaxy presents a largely smooth and rounded morphology, with a concentrated central bulge. The light distribution appears relatively uniform, lacking prominent spiral arms or other distinct features typically associated with disk galaxies. The galaxy exhibits a yellow-orange hue, suggestive of an older stellar population and lower levels of on-going star formation. The absence of pronounced disturbances or tidal tails indicates a relatively isolated system, undisturbed by recent major merger events. There are no obvious signs of an active galactic nucleus.
