The galaxy presents as a somewhat elongated, lenticular structure with a smooth, diffuse appearance, possibly a disk galaxy seen at an angle. It has a prominent central bulge that appears yellowish-orange, suggesting an older stellar population and little to no active star formation. The outer regions show a slight bluer tint and an overall green appearance. This suggests a faint presence of younger, hotter stars, potentially within a flattened disk component. The shape appears moderately elongated, leaning towards a cigar-like structure. There is a suggestion of minor gravitational disturbance or interaction. The galaxy displays an overall undisturbed morphology, without any dominant features indicating a recent major merger event.
