The galaxy presents as a centrally concentrated, elliptical morphology. The light distribution appears smooth with no obvious spiral arm structures or distinct features such as dust lanes or prominent star-forming regions. The color profile is predominantly yellowish-orange in the central region, indicating an older stellar population. There is a subtle hint of greenish hue in the immediate area surrounding the brightest region of the nucleus, this may indicate some star formation may be present in that area. The lack of distinct features suggests a relatively quiescent galaxy, although there are hints of some possible minor disturbance of the galaxy that may imply the possibility of a previous interaction or merger. 
