The galaxy presents a primarily smooth morphology with a concentrated central bulge. It appears elliptical or spheroidal, exhibiting an overall rounded shape, with the majority of light concentrated near the center. There are no obvious spiral arm structures or significant tidal disturbances visible. The galaxy displays a gradual decline in brightness from the core outwards, suggesting a lack of recent major mergers or strong interactions. The color profile is relatively consistent across the galaxy, trending towards redder hues which could be indicative of an older stellar population and lower levels of active star formation. There is a hint of more bluer colors in its outskirts suggesting the possibility of the small occurrence of younger stars.
