The galaxy presents as a somewhat smooth, centralized mass of light. The luminosity is concentrated towards the center with a slight elongation, hinting at an elliptical morphology. The object appears to be generally round and has a yellow hue, potentially indicating an older stellar population. There's some evidence of interaction or disturbance in the galaxy's morphology. The overall structure suggests a relatively quiescent galaxy with a significant mass, likely past its peak star formation. The color implies relatively low current star formation. There is a hint of possible merging event occurring, though the galaxy has settled into its final form.
