The galaxy presents an elliptical morphology, appearing mostly smooth with a concentrated central bulge. The light distribution suggests a lack of prominent spiral arms or significant star-forming regions. The galaxy exhibits a generally rounded shape but has some features that make it slightly more akin to being between round and cigar shaped. There is a hint of some minor disturbance. It appears to be a relatively isolated system with no other prominent galaxies in the immediate vicinity to suggest a major merger. Based on its color indices, the galaxy appears to have a high mass and a relatively low star formation rate.
