The galaxy presents an overall elliptical morphology, elongated along its major axis. The light distribution appears smooth and centrally concentrated, indicative of an older stellar population. A slight asymmetry is visible, possibly due to a minor tidal interaction or internal dust obscuration. There is some hint of bluer light at one side of the galaxy indicating some recent star formation might be occurring. The galaxy lacks any prominent spiral arm structure or a distinct bulge component, suggesting it is likely a lenticular or elliptical galaxy type.
