The galaxy presents as a relatively smooth, elongated structure. Its color profile suggests a predominantly older stellar population with a central concentration of light indicating a bulge or core. Faint blue hues are present on the edges of the galaxy implying there is some ongoing, albeit limited, star formation activity. There is no obvious dust lane or spiral structure. There is no indication of significant tidal disturbance or interaction with neighboring galaxies. Based on the observed morphology, the galaxy can be classified as an elliptical or lenticular galaxy.
