The galaxy presents a generally smooth, elliptical morphology. It has a bright, concentrated central bulge exhibiting a reddish hue, indicative of an older stellar population. There is a discernible disk component with a slight inclination relative to our line of sight. The disk demonstrates subtle color gradients, transitioning from greenish-yellow tones closer to the central bulge to bluer tones further out, suggesting ongoing star formation in the outer regions. There is a single noticeable, bright red region, likely an area of high star formation, located off-center. Overall, the galaxy appears to be a relatively massive system with a combination of evolved and actively star-forming regions. A degree of interaction or merger is suggested by the subtle disturbances in its overall structure.
