The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. Fainter, bluer regions extend from the central bulge, possibly indicating areas of more recent, albeit modest, star formation. The galaxy lacks any prominent spiral arm structure or obvious signs of a major ongoing merger event. There's a slight asymmetry in the outer regions of the galaxy, possibly hinting at a minor interaction or past disturbance. Overall, the galaxy appears to be a fairly massive system with moderate star formation.
