The galaxy presents as a diffuse, centrally concentrated object with a slightly elongated morphology, possibly disk-like. There appears to be some indication of interaction or disturbance in the form of asymmetry and/or tidal features. The color profile suggests a mix of stellar populations, with a faint blueish tinge in the outer regions that could indicate some low levels of on-going star formation. A significant proportion of the light seems to be emitted from older stellar populations within the central region, which give it a relatively smooth appearance. Overall the galaxy presents faint and disturbed structure.
