The galaxy presents an overall smooth morphology, suggesting it is an early-type galaxy, potentially an elliptical or lenticular. The central region exhibits a concentrated, bright bulge with a yellowish hue, indicative of an older stellar population. There is a very subtle disk-like component, displaying a slight flattening and bluer color than the central bulge, suggesting some ongoing, though subdued, star formation activity. The overall shape is somewhat elongated, appearing cigar-shaped. There is no obvious evidence of spiral arms, tidal tails, or major disturbances, suggesting it is not currently undergoing a major merger event. The color gradient from the center outwards indicates a decreasing age of stellar populations. The galaxy appears to be a relatively massive system with a moderate rate of star formation.
