The galaxy presents an elliptical morphology, appearing elongated along one axis. Its core exhibits a concentrated luminosity, suggesting a high stellar density. The light profile appears relatively smooth with a fading gradient as it extends outward from the central bulge. The color distribution shows a yellowish-white hue in the core, possibly indicating an older stellar population, with hints of bluer tints on the outer edges of the disk, implying some ongoing star formation. There is no apparent spiral arm structure or bar. No significant dust lanes or tidal features are visible, implying a relatively quiescent state. Overall, the galaxy appears to be a massive system.
