The galaxy presents as a slightly elongated, lenticular-like structure. The light distribution appears smooth, with no distinct spiral arms or prominent dust lanes visible. The central region exhibits a brighter, more concentrated luminosity, suggesting a galactic bulge. There is a gradual decrease in surface brightness from the core outwards. The overall color appears to be dominated by yellow-red hues. The galaxy exhibits a high probability of not being currently undergoing merging activity. It has a relatively moderate amount of star formation present. The approximate estimated average mass of the stars within this galaxy is calculated to be approximately 10^9.8 Solar Masses.
