The galaxy exhibits a predominantly smooth morphology, suggesting a relatively evolved system. It appears as an elliptical or lenticular type, with a lack of strong spiral arm structures. There is some visual evidence of internal structure within the galaxy, with an area of slightly brighter luminosity near the center. This is most likely due to a bulge containing a dense stellar population. There appears to be some minor visual disturbances in the galaxy's overall shape, potentially indicative of a past or ongoing interaction with a smaller companion galaxy. The color profile suggests a relatively older stellar population.
