The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The color profile is dominated by redder hues, indicative of an older stellar population. There is a lack of discernible spiral arm structure. There are no obvious indications of active star formation regions. The galaxy does not appear to be undergoing any major merging events or significant disturbances. The overall morphology suggests a galaxy nearing the end of its star forming era, potentially transitioning into a quiescent state.
