The galaxy appears as a moderately bright, elliptical-shaped structure, displaying a smooth and centrally concentrated morphology. There is a noticeable color gradient, transitioning from a more yellowish hue at the core to a slightly bluer periphery, suggesting ongoing star formation is present but is likely more pronounced in the outer regions. The galaxy shows little evidence of spiral arm structure, and appears to be undergoing some sort of merger or tidal disturbance. Several luminous regions are visible, possibly indicative of star clusters or active galactic nuclei. The size of the galaxy is relatively moderate, indicating a potentially substantial, although not extremely large, mass. There appears to be some surrounding loose material as well.
