The galaxy presents as a generally smooth object with a slight ellipticity, appearing more akin to a disk galaxy, though with possible subtle features. It does not show any obvious signs of major mergers or significant tidal disturbances. The galaxy exhibits a color gradient, being bluer in the central region and gradually becoming redder toward the outskirts. This color variation suggests a possible difference in stellar populations, with a higher concentration of younger, hotter stars in the core, and older, cooler stars dominating the outer regions. The galaxy's overall color profile indicates a relatively low rate of ongoing star formation. Its size is consistent with a galaxy of moderate physical dimensions.
