The galaxy presents an elliptical morphology, appearing elongated with a cigar-shaped profile. Its overall structure suggests a smooth distribution of light, with a concentrated central bulge. The light from the galaxy exhibits a color gradient, transitioning from a yellowish hue in the core to a slightly bluer tint towards the outer edges. This color variation could imply differing stellar populations and ages across the galaxy. There is no clear evidence of spiral arms, significant dust lanes, or ongoing major merger activity. Instead, a subtle irregularity in the outer regions may point toward a minor disturbance or past interaction. The estimated size indicates that it is a relatively large galaxy. The overall characteristics suggest that the galaxy is a relatively massive system, and is experiencing some star formation.
