The galaxy presents as a singular, relatively smooth structure. The overall color profile is dominated by redder hues, suggesting an older stellar population. It appears largely spheroidal, with no discernible spiral arm structure or prominent disk. There are hints of some irregular features or minor disturbances in its morphology. There appears to be a low rate of ongoing star formation, with only minor indicators of bluer regions. The galaxy appears fairly massive, with what can be roughly considered to be average to low rate of star formation for this size of galaxy.
