The galaxy presents as a relatively smooth, elliptical-like structure with no apparent spiral arms or strong disk features. The light distribution is concentrated towards the center, suggesting a prominent galactic nucleus. The overall color appears to be a yellowish-orange hue, which is consistent with an older stellar population and potentially lower rates of current star formation. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The galaxy exhibits a moderately concentrated morphology, appearing generally round but with some deviation from perfect circularity. There may be some faint signs of minor disturbances in the galaxy, however there are no other signs of it merging.
