The galaxy presents as a relatively smooth object, exhibiting a slightly elongated, rounded morphology. It shows a concentration of light towards the center, suggesting a bulge. There is some possible evidence of a minor tidal disturbance or asymmetry in the overall structure, which may suggest a past or ongoing interaction with another galaxy. There is a secondary object to the south of the galaxy that is smaller and dimmer, it is unclear if this is another galaxy or simply a foreground object.
The galaxy displays a color profile that indicates it is likely composed of an older stellar population with low ongoing star formation.
