The galaxy presents as a generally smooth, elliptical-like structure. The central bulge exhibits a bright, concentrated core that appears roughly circular. There is a gradual decrease in surface brightness moving outwards from the core, without any pronounced spiral arms or distinct features. The overall color of the galaxy leans towards the redder end of the spectrum, indicative of an older stellar population with lower rates of current star formation. There may be a slight dust lane obscuring one side of the galactic disk, suggesting a relatively small amount of recent merger activity. The galaxy appears relatively isolated with no visually apparent major interactions or merging events occurring with nearby galaxies.