The galaxy presents as an elliptical morphology. It exhibits a generally smooth light distribution, lacking any immediately obvious spiral arm structures or prominent dust lanes. The core is relatively bright and concentrated, suggesting a significant stellar density. The shape appears more in-between round and cigar shaped. There is a slight color gradient, with the central bulge tending toward yellow and the outer regions exhibiting a more complex color profile. The overall appearance suggests a relatively evolved system with a low current star formation rate. There is no indication of major merging events.
