The galaxy presents a generally smooth and rounded morphology, with no distinct spiral arms or bar structure evident. The primary color appears to be yellow-reddish, which indicates an older stellar population with fewer active star-forming regions and a higher concentration of evolved stars. The absence of blue-ish colors, typically associated with young, hot stars, further supports this. There is no obvious dust lane or significant obscuration. The galaxy has a concentrated core, with a gradual decrease in surface brightness towards its outer regions. There are no apparent signs of major disturbances such as tidal tails or strong asymmetries, suggesting that it is not currently undergoing a major merger. However, the suggestion of multiple distinct points of light within the galaxy's extended halo may indicate some minor interactions or small satellite galaxies being accreted.
