The galaxy presents as a relatively smooth, centrally concentrated object, appearing almost elliptical in shape. There is little evidence of spiral arm structure or distinct features that would suggest a disk-dominated system. The core of the galaxy exhibits a bright, diffused luminosity, decreasing in intensity toward the outer regions. There is a slight elongation or asymmetry that may indicate some minor gravitational interaction or internal disturbance. Overall, the galaxy’s morphology suggests a relatively evolved system, possibly an early-type spiral or elliptical. A potential companion galaxy appears to the side, suggesting possible merging activity, but there is no conclusive evidence of major tidal disruption or strong interaction between the two systems. The color appears to be generally red, possibly indicating an older stellar population and lower ongoing star formation activity.
